Category Astronomy

How long does it take the International Space Station to orbit the Earth ______ minutes?

The International Space Station (ISS) is a large spacecraft that orbitis around Earth every 90 minutes. It is not only a science laboratory but also serves as a home to crews of astronauts and Cosmonauts.

Its laboratory has components from the United States, Russia, Japan, and Europe.

The space station is used by National Aeronautics and Space Administration (NASA) scientists to learn more about living and working in space. The research here will make it possible to send humans farther into space than ever before.

History                                                                                               

Originally called ‘Freedom’ in the 1980s, then U.S. President Ronald Reagan authorised NASA to build the space station. It was redesigned in the 1990s to reduce costs and expand international involvement, at which time it was renamed.

In 1993, the U.S. and Russia agreed to merge their separate space station plans into a single facility and incorporate contributions from the European Space Agency (ESA) and Japan.

It took 10 years and more than 30 missions to assemble the space station. It was launched in 1998 with the help of the U.S., Russia, Canada, Japan, and the participating countries of the ESA. The first piece of the ISS was launched in November 1998. The ISS is the size of a large five-bedroom house or a football field and is able to support a crew of six people and some visitors

It is made up of several parts that were assembled in space by astronauts. The first crew reached the space station on November 2, 2000. People have lived on the space station ever since.

International Space Station

The space station is equal to a five-bedroom house or the size of a football field and is able to support a crew of six people, plus visitors. The laboratories in the space station help the crew members to do research that could not be done anywhere else.

At the ISS, the scientists also study what happens to the human body when people live in microgravity (place where there is almost no gravity) for a long time.

The space station has solar arrays, which collect energy from the sun to provide electrical power. The arrays are connected to the station with a long truss, which is a beam that is the backbone of the space station.

There are radiators on the truss that control the space station’s temperature. Astronauts reach the space station on the Russian Soyuz spacecraft Operating the space station is more complicated than other space flight programmes as it is an international programme. Each partner is mainly responsible for managing and running the hardware it provides It is the largest space station ever constructed and yet it continues to be assembled in orbit.

Till now, it has been visited by astronauts from 18 countries During Prime Minister Narendra Modi’s recent visit to the U.S.. President Joe Biden said that India and the US. will collaborate to send an Indian astronaut to the ISS in 2024.

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Does Saturn have a storm spot?

The Great Red Spot is the largest storm in our solar system. An anticyclone that is over 16,000 km wide-large enough to engulf the entire Earth-the Great Red Spot has been on Jupiter’s surface for hundreds of years.

A new study has shown that Satum Jupiters neighbour, also has long-lasting megastorms. While these are less colourful and blander than those on Jupiter, they do have impacts deep in Saturn’s atmosphere that remain for centuries. The study was published on August 11 in the journal Science Advances

Similar to hurricanes

Similar to hurricanes on Earth but much much larger, megastorms on Satum occur every 20 to 30 years. The causes for these megastorms in Saturn’s atmosphere. which is made up mainly of hydrogen and helium along with traces of methane ammonia and water, remains unknown. Based on radio emissions from Satum. astronomers from the University of California, Berkeley, and the University of Michigan, Ann Arbor, noticed anomalies in the concentration of ammonia gas in the atmosphere. While the concentration of ammonia at mid-altitudes is lower, it was enriched at lower altitudes. 100 to 200 km deeper in the atmosphere.

Precipitation and re-evaporation

The researchers were able to connect this to the past occurrences of megastorms in Satum’s northern hemisphere. According to them, ammonia is being transported from the upper to the lower atmosphere. This effect, which they believe can last for hundreds of years, occurs through the processes of precipitation and re-evaporation.

Additionally, this study reveals that Saturn and Jupiter are very dissimilar despite the fact that both gas giants are made of hydrogen gas. The tropospheric anomalies in Jupiter have been connected to its zones (whitish bands) and belts (darkish bands), while those on Saturn are caused by cyclones.

These differences between Saturn and Jupiter challenge scientists on what they know about the formation of megastorms on gas giants and other planets. Understanding this would not only further our knowledge of terrestrial meteorology, but may also inform us as to how they are formed and studied on exoplanets in the future.

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What will replace the ISS in 2031?

The International Space Station or ISS is to be deorbited by 2031. Where will it go? Satellites and spacecraft are machines, similar to washing machines and vacuum cleaners. They will not last forever. It doesn’t matter what job they do, whether it’s to observe weather, measure greenhouse gases in the atmosphere, or study the stars. All space machines grow old, wear out and die.

For satellites in Low Earth Orbit (LEO), engineers use the last bit of fuel to slow it down. When the fuel runs out, it falls out of orbit and burns up in the atmosphere. The satellites in very high orbits are sent even further away from Earth, since more fuel is required to bring them down! These satellites are sent into a so-called ‘graveyard orbit, almost 36,000 km above Earth. Space stations and large spacecraft that are in LEO are too large to incinerate entirely on re-entry. So the deorbiting is monitored closely to ensure the debris falls on a remote, uninhabited area. There is an area like this. It’s nicknamed ‘spacecraft cemetery’ and it lies in the middle of the South Pacific Ocean at a spot called Point Nemo. (‘Nemo’ is Latin for ‘nobody’.) Point Nemo is so remote that the ISS will meet its watery grave there. It is considered ideal for dumping space debris as the waters are said to be poor in nutrients and biodiversity. No one has really studied the marine life or lack of it in Point Nemo. Environmentalists fear that in addition to the space junk already present in Point Nemo, the ISS debris will add tons of experimental equipment, materials and even traces of altered human DNA.  

Who was the first person to float freely in space?

Images from space that show earth as nothing more than a blur of blue tug at our hearts in a way that can’t be put into words. The ones that you see here, while evoking such emotions, are also iconic in their own right. This is because they show the first human ever to walk untethered in space. The subject of these photographs is NASA astronaut Bruce McCandless II.

Born in Boston in 1937, McCandless did his schooling at Long Beach, California and received his Bachelor of Science degree from the United States Naval Academy in 1958. He then obtained his Master of Science degree in Electrical Engineering from Stanford University in 1965, and eventually also ended up with a Masters in Business Administration from the University of Houston in 1987.

Communicator role

A retired U.S. Navy captain, McCandless was one of 19 astronauts selected by NASA in April 1966. He served as the mission control communicator for Neil Armstrong and Buzz Aldrin during their famous 1969 Apollo 11 mission, which included the first human landing on the moon. McCandless, in fact, famously felt let down by Armstrong as the latter hadn’t revealed ahead what he had planned to say while setting foot on the moon.

McCandless flew as the mission specialist on two space shuttles, STS-41B in 1984 and STS-31 in 1990. While the 1984 mission saw him become the first human to perform an untethered spacewalk, he helped deploy the Hubble Space Telescope during the 1990 mission.

Helps develop MMU

Apart from these, McCandless also served as a member of the astronaut support crew for the Apollo 14 mission and was a backup pilot for the first crewed Skylab mission. For the M-509 astronaut manoeuvring experiment that was flown in the Skylab programme, McCandless was a co-investigator. He collaborated on the development and helped design what came to be known as the MMU – manned manoeuvring unit.

The STS-41B was launched on February 3, 1984. Four days later, on February 7, McCandless stepped out of the space shuttle Challenger into nothingness. As he moved away from the spacecraft, he floated freely without any earthly anchor.

“Heck of a big leap for me”

“It may have been a small step for Neil, but it’s a heck of a big leap for me,” were McCandless’ first words. If the mood at mission control had been apprehensive before, the raucous laughter that followed this comment certainly reduced the tension – a fact that was confirmed by his wife, who was also at mission control. McCandless would later say that his comment was consciously thought out and that it was his way of saying things were going okay, apart from getting back at Armstrong for not revealing his words in 1969.

The images that were shot then, showing McCandless spacewalking without tethers, gained widespread fame. The spacewalk was the first time the MMU that he helped develop was used. These nitrogen-propelled, hand-controlled devices afforded much greater mobility to their users as opposed to restrictive tethers used by previous spacewalkers.

Fellow astronaut Robert L. Stewart later tried out the MMU that McCandless first used. Two days later, both of them tried another similar unit with success. By February 11, the STS-41B mission was complete as the Challenger safely landed at NASA’s Kennedy Space Centre.

In one of his last interviews, before his death in December 2017, McCandless told National Geographic what he had probably told countless others who wanted to know how it was out there.

Fun, but cold

While he always maintained that it was fun, he also adds that the single thing that disturbed him as he moved away from the shuttle was that he got extremely cold, with shivers and chattering teeth.

The reason for that is pretty straightforward. While he had prepared for that moment for years, he wasn’t prepared for the temperature in the suit. As the suit was designed to keep astronauts comfortable while working hard in a warm environment, even the H (hot) position on the life support system actually provided minimal cooling. Considering that McCandless wasn’t really performing strenuous labour during the first hours of his untethered spacewalk, he felt cold. That’s a small price to pay for becoming the first-ever human to walk freely in space.

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What powers a spacecraft?

Scientists send spacecraft to probe objects in space. These spacecraft carry instruments that help them take pictures and collect data in space and send them back to Earth. But to do this, the spacecraft needs electricity So what powers it?

Based on the mission it is assigned, and factors such as where the spacecraft is travelling, what it plans to do there and how long it needs to work engineers choose the best way to power a spacecraft.

The Sun                     

One source of power engineers consider is energy from the Sun, or solar power. Spacecraft that orbit close to Earth are dose enough to the Sun to use solar power. These spacecraft are fitted with solar panels, which convert the Sun’s energy into electricity. The electricity from the panels charges a battery in the spacecraft and can be used even when the spacecraft doesn’t have direct sunlight

Batteries

Sometimes, when the mission is only for a short duration, such as the Huygens probe that landed on Titan, Saturn’s largest moon, and meant to work only for a few hours, engineers may power the spacecraft with batteries. These batteries are designed to be tough since they need to withstand the harsh environment of space.

Atoms

An atom is a tiny building block of matter. Atoms need to store a lot of energy to hold themselves together. However, atoms such as radioisotopes are unstable and begin to fall apart. As they fall apart, they release energy as heat. A radioisotope power system uses the temperature difference between the heat from the unstable atoms and the cold of space to produce electricity. This system produces power for a very long time even in harsh environments. That’s why this system has been used to power many of NASA’s missions, including the two Voyager spacecraft that continue to send back information after over four decades in space.

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What is the streak of light that shoots across the night sky called?

During Earth’s journey around the Sun, there are times when its orbit crosses the orbit of a comet. It is when the planet moves through the comet debris trail that we witness meteor showers. The showers are named after the star or constellation which is close to where the meteors appear to radiate in the sky.

All of us may have seen streaks of light zip through the sky. We call them shooting stars and we also wish upon them. Well, what are these shooting stars? What are these streams of light? Consider the objects in space. These are lumps of rock or objects in space with sizes ranging from grains to small asteroids. A small piece of a comet or asteroid is called a meteoroid.

Meteoroid

These meteoroids can be considered as space rocks. They orbit the sun and when they enter Earth’s atmosphere at a high speed, they burn because of frictional heating, causing the light. These rays of light are referred to as meteors.

When many meteors appear at once, we call it a meteor shower. During a meteor shower, a number of meteors can be seen radiating or originating from a point in the night sky.

But where do these meteoroids come from? How does Earth come across these? During Earth’s journey around the Sun, there are times when its orbit crosses the orbit of a comet. It is when the planet moves through the comet debris trail that we witness meteor showers.

The meteor showers are named after the star or constellation which is close to where the meteors appear to radiate in the sky. The Perseids meteor shower is the most famous meteor shower and they peak around August 12 every year. Other notable meteor showers include the Leonids, Aquarids and Orionids and Taurids.

Now what happens when meteoroid survives the journey through the Earth’s atmosphere and hits the ground? In that case, it becomes a meteorite.

Did you know that more than 50,000 meteorites have been found on Earth?

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Are Membrane mirrors for large space-based telescopes?

Researches create lightweight flexible mirrors that can be rolled up during launch and reshaped precisely after deployment.

Mirrors are a significant part of telescopes. When it comes to space telescopes, which have complicated procedures for launching and deploying, the primary mirrors add considerable heft, contributing to packaging difficulties.

Researchers have now come up with a novel way of producing and shaping large, high-quality mirrors. These mirrors are not only thinner than the primary mirrors usually employed in space-based telescopes, but are also flexible enough to be rolled up and stored inside a launch vehicle.

Parabolic membrane mirror

The successful fabrication of such parabolic membrane mirror prototypes up to 30 cm in diameter have been reported in the Optica Publishing Group journal Applied Optics in April. Researchers not only believe that these mirrors could be scaled up to the sizes required in future space telescopes, but have also developed a heat-based method to correct imperfections that will occur during the unfolding process.

Using a chemical vapour deposition process that is commonly used to apply coatings (like the ones that make electronics water-resistant), a parabolic membrane mirror was created for the first time. The mirror was built with the optical qualities required for use in telescopes. A rotating container with a small amount of liquid was added to the inside of a vacuum chamber in order to create the exact shape necessary for a telescope mirror. The liquid forms a perfect parabolic shape onto which a polymer can grow during chemical vapour deposition, forming the mirror base. A reflective metal layer is applied to the top when the polymer is thick enough, and the liquid is then washed away.

Thermal technique

The researchers tested their technique by building a 30-cm-diameter membrane mirror in a vacuum deposition chamber. While the thin and lightweight mirror thus constructed can be folded during the trip to space, it would be nearly impossible to get it into perfect parabolic shape after unpacking. The researchers were able to show that their thermal radiative adaptive shaping method worked well to reshape the membrane mirror.

Future research is aimed at applying more sophisticated adaptive control to find out not only how well the final surface can be shaped, but also how much distortion can be tolerated initially. Additionally, there are also plans to create a metre-sized deposition chamber that would enable studying the surface structure along with packaging unfolding processes for a large-scale primary mirror.

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Which was the first successful soft landing on Mars?

Launched on May 28, 1971, Mars 3 was one among a pair of identical spacecraft. While its lander stopped transmitting data after less than 20 seconds, it nevertheless represents the first successful soft landing on Mars. A.S.Ganesh hands you the details about the Mars 3 mission…

When we talk about the space race between the Cold War adversaries the US. and the Soviet Union, we usually discuss the race to land the first human beings on the moon. Soon after this was achieved, however, attention shifted to our neighbouring planet Mars. The first successful soft landing on Mars was achieved by the Soviet Union with their Mars 3 mission.

At this initial period of planetary exploration, both these space superpowers tended to launch pairs of spacecraft as a precautionary measure. The idea was to have one as the backup. of another, so that at least one of them succeeded in its efforts even if the other failed completely in its objective.

It therefore comes as no surprise that the Mars 2 and Mars 3 missions consisted of identical spacecraft. With a bus/orbiter module and an attached descent/lander module, the combined mass of the spacecraft, with fuel, was approximately 4,650 kg. The Mars 3 spacecraft was 4.1 metres high. 5.9 metres across the two solar panel wings and had a base diameter of 2 metres.

Primary objectives

The primary objective of the Mars 3 orbiter was to image the martian surface and clouds. determine the temperature on Mars, and measure properties of the martian atmosphere. among others. These were in addition to serving as a communications relay to send signals from the lander to Earth.

Mars 3 was launched on May 28, 1971, just nine days after Mars 2 had been successfully launched. Ten days later, on June 8, a mid-course correction was made after which Mars 3 was involved in a three-way race with Mars 2 and U.S.’ Mariner 9 to become the first spacecraft to orbit Mars.

Even though Mariner 9 was last off the blocks, having been launched on May 30, it became the first to reach Mars on November 14. Mars 2 reached Mars on November 27 and Mars 3 made it to its destination on December 2.

Achieves soft landing

 Less than five hours before reaching Mars, the descent module of Mars 3 had been released. Having entered the martian atmosphere at roughly 5.7 km/s, a combination of aerodynamic braking, parachutes, and retro-rockets allowed the lander to achieve a soft landing. With the Mars 2 lander having crashed, this made the Mars 3 mission the first ever to achieve a soft landing on Mars.

Only just though, as the lander stopped transmitting and the instruments stopped working less than 20 seconds after the successful landing. While the reasons remain unknown, the massive surface dust storms that were raging at the time of landing could have caused the lander to stop working.

As the orbiter had suffered a partial loss of fuel, it couldn’t put itself into the planned 25 hour orbit. Instead, a truncated burn was performed by the engine in order to put the spacecraft into a 12 day, 19 hour long orbit about Mars.

20 orbits around Mars

A large volume of data was sent hack by Mars 2 and Mars 3 orbiters from December 1971 to March 1972, even though transmission continued till August. On August 22, 1972, an announcement was made stating that Mars 2 and Mars 3 had completed their missions. While Mars 2 had completed 362 orbits of the red planet, Mars 3 had performed 20 orbits.

Apart from the 60 images received from the probes, the data provided by them revealed mountains as high as 22 km, atomic hydrogen and oxygen in the upper atmosphere, and surface temperatures and pressures. The data gathered not only provided information on the martian gravity and magnetic fields, but also helped create surface relief maps.

Mars 3 was back in the news four decades later in April 2013 when citizen enthusiasts found features of its hardware in a five-year-old image from NASA’s Mars Reconnaissance Orbiter. The debris in the images resembled what might have been the parachute, heat shield, terminal retrorocket and lander. Regardless of whether these were the debris of the Mars 3 lander or not, the mission did successfully become the first ever to achieve a soft landing on our neighbouring red planet.

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What are the Astronomers, who helped enhance our understanding of the cosmos?

We have always been looking up, peering into the sky, trying to find answers to the many questions about the universe. Many astronomers have tried to unravel the mysteries of the universe. From believing that Earth was flat and the planets revolved around it, we have come a long way. Let’s take a look at some of history’s greatest astronomers who helped enhance our understanding of the Cosmos.

From believing that the Earth was flat and the planets revolved around it, we have come a long way.Some 2000 years ago, when it was widely believed that the world was flat, Greek mathematician and astronomer Eratosthenes (276 BC-194 BC) calculated the Earth’s circumference. In those days, the very act of coming up with scientific thoughts which were at odds with the ones in existence was not encouraged. The theory that the Earth revolved around the Sun was itself considered heretical by the religious and after a trial, Italian astronomer Galileo Galilei was kept under house arrest until his death. Polish astronomer Nicolaus Copernicus didn’t publish his magnum opus “De revolutions orbium coelestium” (On the Revolutions of the Heavenly Spheres) until he was on his deathbed. Let’s take a look at some of history’s greatest astronomers who threw new light on the cosmos.

CLAUDIUS PTOLEMY (AD 100-AD 170)

 Astronomer and mathematician Claudius Ptolemy authored several scientific teas and is noted for his Ptolemaic system. It was a geocentric (Earth-centred) model of the universe, where the sun, stars, and other planets revolved around Earth. This model was used for a long period, for over 1200 years, until the heliocentric view of the solar system was established. Although his model of the universe was wrong, his work and the scientific texts he authored helped astronomers make predictions of planetary positions and solar and lunar eclipses. “The Almagest, a comprehensive treatise on the movements of the stars and planets, was published in the 2nd Century. It is divided into 13 books. This manual served as the basic guide for Islamic and European astronomers. He also catalogued 48 constellations. 

NICOLAUS COPERNICUS (1473-1543)

 Nicolaus Copernicus changed the way scientists viewed the solar system. Back in the 16th Century, he came up with a model of the solar system where the Earth revolved around the Sun: it was the revolutionary heliocentric model. He removed Earth from the centre of the universe and replaced it with the Sun! He also didn’t believe in the Ptolemaic model of the planets travelling in circular orbits around the Earth. He also explained the retrograde motion of the planets (retrograde motion is when planets appear to move in the opposite direction of the stars). When the Polish astronomer was 70, he published his book “De Revolutions Orbium Coelestium” (“On the Revolutions of the Heavenly Spheres”), on his deathbed. It took over a century for his idea to gain credence.

GALILEO GALILEI (1564-1642)

Optical astronomy began with Galileo Galilei. Born in Italy, Galilei is credited with creating the optical telescope. In fact, what he did was improve upon the existing models. He came up with his first telescope in 1609, modelling it after the telescopes produced in other parts of Europe. But here is the catch. Those telescopes could magnify objects only three times. Galileo came up with a telescope that could magnify objects 20 times. He then pointed it towards the sky, coming up with the greatest discoveries ever. He discovered the four primary moons of Jupiter which are referred to as the Galilean moons. He also discovered the rings of Saturn. Even though the theory of Earth circling the Sun had been around since Copernicus’ time, when Galileo defended it, he was kept under house arrest till the end of his lifetime.

JOHANNES KEPLER (1571-1630)

Danish astronomer Johannes Kepler modified the Copernican view of the solar system and changed it radically. He deduced that the planets travelled in elliptical orbits, one of the most revolutionary ideas at the time, replacing Copernicus view that they travelled in circular objects. He came up with three revolutionary laws involving the motions of planets these three laws make him a towering figure in astronomy. Kepler also observed a supernova in 1604. It is now called Kepler’s Nova.

EDMOND HALLEY (1656-1742)

“Halley’s comet is perhaps a term you would have heard quite often. English astronomer Edmond Halley never saw the comet named after him. Officially called 1P/Halley, Halley’s  comet  is a periodic comet that passes by the Earth once every 76 years (roughly). This famed comet will return in 2061. It was Halley’s mathematical prediction of the comet’s return that made him a towering figure among the list of astronomers. He said that the comet that appeared in 1456, 1531, 1607, and 1682 were all the same and that it would return in 1758. Halley was never around to witness this, but the world saw the comet and its return. The comet was later named in his honour. One of the earliest catalogues of the southern sky was also produced by Halley. In 1676, he sailed to the island St. Helena, South Atlantic Ocean. There he spent a year measuring the position of stars and came up with the first catalogue of the southern sky! Seen here is a painting of the astronomer. 

WILLIAM HERSCHEL (1750-1848)

Musician-tumed astronomer William Herschel started exploring the skies with his sister Caroline quite late in his career but eventually, he compiled a catalogue of 2.500 celestial objects The German astronomer discoverest the planet Uranus and several moons of other planets it was during his mid 30s that he startet looking up and exploring the cosmos In 1759. Herschel left Germany and moved to England where he started teaching music When Herschels interest in astronomy grew, rented a telescope. He then went ahead and built himself a large telescope to watch the celestial bodies. His sister Caroline assisted him until Herschel’s death and also became the first woman to discover a comet. She eventually discovered eight of them. When Herschel found a small object in the night sky, he explored further and found out that it was a planet. The Uranus was thus discovered. He was knighted by the monarch after the discovery and was appointed the court astronomer. Following this he gave up his music career and devoted himself to the skies. He found the moons of Uranus and Saturn Craters on the moon. Mars and Mimas (Saturn’s moon) are named after the astronomer.

ANNIE JUMP CANNON (1863-1941)

Known as the “census taker of the sky, American astronomer Annie Jump Cannon made stellar contributions to the field of astronomy. She classified around 3,50,000  stars manually. At a time when gender representation in astronomy was  skewed. Cannon with her impeccable contributions inspired many women to pursue astronomy. During that time, stars were classified alphabetically, from A to Q. based on their temperatures. She built a new classification system with ten categories and forever changed the way scientists classified stars by developing the Harvard system which is in use even today.

CARL SAGAN (1934-1996)

American astronomer Carl Sagan was not just a science poster boy but he was one of the most influential voices in the scientific  realm  who  made the cosmos a subject of interest for the masses. Sagan played a huge role in in the American space program. He popularised astronomy and through his talks and books motivated many to become sky watchers. He also founded the Planetary Society, a non-profit that is focussed on advancing space science and exploration. He was a professor of astronomy and space sciences and director of the Laboratory for Planetary Studies at Cornell University. His contributions include explaining the high temperatures of Venus and the seasonal changes on Mars. His book “Cosmos” is a bestseller that was also turned into a television show (hosted by Sagan) which was watched by a billion people in 60 countries. He also wrote a science fiction novel “Contact” which was adapted to the screen.

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What is SWOT?

The satellite has been designed to conduct a landmark survey of the world’s oceans, lakes, and rivers from space for the first time.

NASA, the U.S. space agency, recently launched a satellite called SWOT. What is its objective and how will it help us? Let’s find out.

Its mission

SWOT, short for the Surface Water and Ocean Topography satellite, was recently launched from California to make a comprehensive survey of the world’s oceans, rivers, and lakes from space for the very first time. Dubbed a “revolution in hydrology”, SWOT, an SUV-sized satellite flying at a height of 890 km, will offer an unprecedented, clear view of the water bodies, while tracking the rise in sea levels, as well as rivers, lakes, and reservoirs. The satellite is expected to offer key insights into how these bodies of water influence climate change and factors such as how much more heat and carbon dioxide oceans can absorb. Oceans are estimated to have absorbed more than 90% of the excess heat trapped in Earth’s atmosphere caused by human-induced greenhouse gas emissions. With climate change accelerating, some regions are experiencing extreme droughts. while others extreme floods, along with changing precipitation patterns. According to researchers, the observations of SWOT will improve our understanding of how water moves around Earth, its circular currents in oceans, etc. This will help predict floods in areas where there is too much water, and manage water in places that are prone to drought.

How will it work?

The global water survey satellite will measure the height of water in freshwater bodies and the ocean on more than 90% of Earth’s surface – which it will track at least once every 21 days. Researchers will be able to get data on millions of lakes, rather than the few thousands currently visible from space. The technology employed by SWOT is called KaRin, a Ka-band radar interferometer. The radar sends down a signal which is reflected back by the water surface. This echo is received by two antennas, resulting in two sets of data providing high accuracy for water detection and resolution. The data, compiled from the radar sweeps of the planet, will be used to bolster weather and climate forecasts and aid in managing scarce freshwater supplies in drought-stricken areas.

Who developed it?

The satellite is a billion-dollar project developed jointly by NASA and France’s space agency CNES, with contributions from the Canadian space agency and the U.K. space agency. It was carried onboard a spacex Falcon-9 rocket from the Vandenberg U.S. Space Force Base. SWOT will start collecting scientific data in about six months time after undergoing checks and calibrations. The satellite’s components were built primarily by NASA’s Jet Propulsion Laboratory near Los Angeles and CNES.

According to SWOT’S project head at CNES, Thierry Lafon, the mission is meant to last for three-and-a-half years, but could be extended. The U.S. and French space agencies have worked together in the field for over three decades. An earlier satellite developed by the two agencies, TOPEX/Poseidon, improved understanding of ocean circulation and its effect on global climate. It also aided the forecast of the 1997-1998 El Nino weather phenomenon.

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What is the significance of Artemis Accord for India?

India’s aspirations in the outer space and acceptance of the Artemis Accords have affirmed the country’s interest in building a greater relationship with the National Aeronautics and Space Administration (NASA) and its partners. As the space community lauds India’s acceptance of the Artemis Accords, let us know more about it.

Artemis Accords

The Artemis Accords are part of the Artemis programme, which is a mega-initiative by NASA with the aim to land the first woman and first person of colour on the Moon, make new scientific discoveries, and explore more of the lunar surface. Artemis is the name of the goddess of the Moon in Greek mythology and also the twin sister of Apollo.

The Artemis Accords were established in 2020 by NASA, the U.S., and seven other founding member nations – Australia, Canada, Italy, Japan, Luxembourg, UAE, and the U.K. This June 21, India became the 27th country to sign the Artemis Accords.

The Artemis Accords are a set of non-binding guidelines designed to guide civil space exploration and use in the 21st Century. It is a NASA-led effort to return humans to the moon by 2025, with the ultimate goal of expanding space exploration to Mars and beyond.

The Artemis Accords reinforce and implement key obligations in the 1967 Outer Space Treaty (which provided the basic framework for international space law). The accords also affirm the importance of the Rescue and Return Agreement opened in 1968, which emphasises the responsibility of nations to safely return astronauts and equipment to Earth.

Besides, the accords emphasise the need to preserve historically significant human or robotics landing sites, artefacts, spacecraft, and other evidence of activity on celestial bodies.

Outer Space Treaty

The Outer Space Treaty is an international treaty binding the parties to use outer space only for peaceful purposes. The treaty was enforced on October 10, 1967, after being ratified by the U.S., then Soviet Union, the U.K.. and several other countries.

The treaty prohibits countries from placing nuclear arms or other weapons of mass destruction in orbit, on the Moon, or on other bodies in space. Also, no country can claim sovereignty over the Moon or other celestial bodies. The countries are liable for any damage caused by objects launched into space from their territory.

India and the Artemis Accords

India’s Indian Space Research Organisation (ISRO) and NASA had been working together in several lunar missions. However, the cooperation was limited to sharing knowledge. With the signing of the Accords, India and the US will share data, technology, and resources, and work together in ensuring the safety and sustainability of exploring the Moon.

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What is the history of heroes?

In the hindi movie Three Idiots, remade in tamil as nanban, a character remarks that the world only remembers those who come first. He says nobody knows the name of the second person to land on the moon, because he is not important. This cannot be farther from the truth. In fact, the person who landed second on the moon in the celebrated hero and, in some accounts, a controversial figure. Interestingly, he was the first person to do something unique in space. Can you name him?

Answer. “Buzz” Aldrin third from left in the above picture, is an American hero, who has made three spacewalks. A Presbyterian elder (elected member of the crurch), Aldrin was the first person to hold a religious ceremony on the moon when he privately took communion. Before he headed into space in 1969, He got special permission to take bread and wine with him to space and give himself communion. He has been accorded numerous honours, including the presidential Medal of Freedom in 1969. Rumours were rife in 2020 that buzz had reported to NASA that he saw aliens on his way to the moon. It was later proven to be false.

In the 1950s, when racial segregation of white and black communities was the norm in the U.S., it was illegal for a black person to sit next to a white person. If a white person had no seat, black passengers had to vacate their seat and offer it. In 1955, one lone black woman passenger refused to abide by this irrational norm. She refused to stand up and offer her seat to a white person, triggering a massive protest that culminated in the U.S. civil rights movement. Can you name this person?

Answer: Rosa Parks was an American civil rights activist who played a crucial role in the Montgomery bus boycott movement. Her actions inspired the local black community in Alabama to organise the movement, which was led by a young Dr. Martin Luther King Jr. Though Parks lost her job as a consequence of her dissent, the U.S. Supreme Court, finally, ruled that bus segregation was unconstitutional. In 1999, Parks was awarded the Congressional Gold Medal, the highest honour the United States bestows on a civilian. Dr. King, of course, went on to become an American hero.

He was nicknamed “Africa’s Che Guevara” for his stance on the West and his fierce anti-colonialist ideology. A military leader, he changed his country’s name from the colonial Upper Volta to Burkina Faso – “the land of honest men”. He initiated several progressive reforms in his country, from promoting vaccinations for babies to banning the horrendous practice of female genital mutilation, and improving access to education. Can you name him?

Answer: Thomas Sankara was a Marxist leader who came to power in 1983 following a leftist coup that overthrew the moderate military faction ruling Burkina Faso. Much like Che Guevara, this frugal-living, motorcycle-riding, guitar-playing leader became a symbol of hope and resistance throughout Africa.

Once, when a reporter asked him why he did not want his pictures hung in public places, he famously said, “because there are seven million Thomas Sankaras here”. A proponent of Pan-Africanism, he was murdered just within four years of coming to power. Sankarism, currently, is a popular political trend in Africa. They believe his murder was orchestrated by imperialist forces.

Bangabandhu, as he is fondly referred to, was a revolutionary who fought for the liberation of East Pakistan. He was the founder of Bangladesh and served as its President and Prime Minister until he and his family were assassinated in 1975. Only two of his daughters, who were abroad at the time, escaped the attack. One of them, Sheikh Hasina, is currently the Prime Minister of Bangladesh. Can you name this leader?

Answer: Sheikh Mujibur Rahman was a socialist revolutionary who was among the leaders of the freedom movement in Bangladesh. Though the leader of a Muslim majority country, Mujib, as he was known among his friends and followers, aspired to build a sovereign and secular country. “First I am a human being, then a Bengali, and after that a Muslim,” he had once famously remarked. Mujib admired Nobel Laureate Rabindranath Tagore’s view that humanism is always greater than nationalism. Many believe his assassination to be linked with his progressive push to develop Bangladesh as a liberal nation. With the assassination of Mujib, Bangladesh slipped into political regression. Secular values of the State degraded gradually and Islam was declared as the State religion in 1988. Persecution of religious minorities became rampant.

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Why does the European Space Agency want to give the Moon its own time?

The European Space Agency announced that space organisations around the world are considering how best to keep time on the moon. The need is for an internationally accepted lunar time zone.

How do you keep track of time on the moon?  What is the lunar reference point? The moon needs to be given its own time zone, the European Space Agency announced recently. As the race to the moon begins and more and more lunar missions are getting deployed, it is become, pertinent to come with a common refer time.

The European Space Agency announced that space organisations and the world are considering how best to keep time on the moon. The idea took out at a meeting in the Netherlands last year in such the participants agreed on the imminent need to set up    “ a common lunar reference time” Pietro Giordana, a navigation system engineer of the space agency said.

“A joint international effort is now being launched towards achieving this, “Giordano said in a statement.

As of now, a moon missions on the time of the country that is operating the spacecraft. The need is for an internationally accepted lunar time zone. This will be easier for all space-faring nations as mare countries and even private companies are aiming for the moon. The NASA is also getting art to send astronauts there.

 The question of time confounded NASA as it was designing and building the international Space Station, fast approaching the 25th anniversary of the launch of its first pierce. The space station doesn’t have its a time zone, But it runs on Coordinated Universal Time, or UTC which is meticulously based on atomic clocks. This ensures in splitting the time difference between NASA and the Canadian Space Agency, and the other partnering space programmes in Russia, Japan and Europe.

Debate is going on among the international team looking into lunar time on whether a single organisation should set and maintain time on the moon.

When it comes to keeping time on the moon, there are technical issues involved. One being that clocks run faster on the moon than on Earth, gaining about 56 microseconds each day, according to the space agency. Also, ticking occur differently on the lunar surface than in bar orbit.

The lunar time will have to be practical for astronauts there, noted the space agency’s Bernhard Hufenbach. NASA is gearing up for its first flight to the moon with astronauts in more than a half-century in 2024, with a lunar landing as early as 2025.

“This will be quite a challenge” with each day lasting as long as 29.5 Earth days, Hufenbach said in a statement. “But having established a working time system for the moon, we can go on to do the same for other planetary destination.” Mars standard Time, anyone?

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What was the first successful airship built by Ferdinand von Zeppelin in 1900?

On July 2, 1900, the first directed flight of the LZ-1, a zeppelin airship, took place in Germany. The man behind it was Ferdinand Graf von Zeppelin, who pioneered the cause of building rigid dirigible airships, so much so that his surname is still popularly used as a generic name.

Aeroplanes are now the norm for air travel but there was a brief period early in the aeronautical history when airships or dirigibles were believed capable of playing a crucial role in aviation development. Large, controllable balloons propelled by an engine, airships are one of two types of lighter-than-air aircraft (the other one being well, balloons of course!)

Now relegated to aerial observations, advertising and other areas where staying aloft is more important than movement, airships come in three main types: the non-rigid airships or blimps, the semi-rigid airships, and the rigid airships, often called zeppelins. The last category is more popular as zeppelins because it was a German man called Ferdinand Graf von Zeppelin who conceived and developed the first rigid dirigible.

Born in Konstanz, Germany on July 8, 1938, Zeppelin studied at the University of Tubingen before entering the Prussian Army in 1858. He travelled to the U.S. during the American Civil War and acted as a military observer for the Union Army.

An idea is born

It was during this time, in 1863, when Zeppelin had the first of several balloon ascensions at St. Paul, Minnesota. While he was quick to realise the weakness of free balloons, their overdependence on winds and their uncontrollability, it was an experience that stayed with him through a lifetime.

By the 1870s, the idea of building a steerable airship had taken shape in Zeppelin’s mind. So when he retired from the army with the rank of brigadier general, he decided to devote himself to building these airships.

Zeppelin toiled for a decade even though there were many naysayers. By 1900, he had built the first rigid-body airship consisting of a long, uniform cylinder with rounded ends. At 420 feet long and 38 feet in diameter, it had a hydrogen gas capacity of nearly 3,99,000 cubic feet.

Flies from a floating hangar

 From a floating hangar on Lake Constance, Germany, the initial flight of LZ-1, the first zeppelin, took place on July 2, 1900. Days away from turning 62, Zeppelin had finally made progress with an idea that had been with him for decades.

While the demonstration wasn’t entirely successful, the craft attained speeds of nearly 32 km/hour, enough to spark enthusiasm around zeppelins, get more donations, and have enough funding to keep the progress happening. Zeppelin tirelessly worked to make new and improved dirigibles and even created the first commercial passenger air service with them by 1910, but it wasn’t until World War I that support from the government finally came in.

With most aeroplanes still in the development phase, the Germans perceived the advantages of zeppelin-type rigid airships, which could not only attain higher altitudes than aeroplanes of the time, but also remain airborne for nearly 100 hours. More than 100 zeppelins were employed by the Germans for military operations during World War I.

Hindenburg disaster

Zeppelin died in 1917, without seeing the heights that his zeppelins reached, and the tragedy that followed. The LZ-127 ‘Graf Zeppelin’ was launched in 1927 and it was one of the largest ever built. Having a length more than that of two-and-a-half football fields, it made a number of trans-Atlantic flights.

The LZ-129 ‘Hindenburg’ came about in 1936 and was touted to become the most famous zeppelin ever. Instead, tragedy struck and the ‘Hindenburg’ exploded and burned on May 6, 1937 at its mooring mast in New Jersey. (In case you were wondering, the Hindenburg Research investment company, which has constantly been in the news this year following their reports about the Adani Group, was named after this zeppelin.)

The Hindenburg disaster spelt doom for zeppelins as the remaining ones were also taken off service and dismantled. While safety concerns diminished their popularity, they had helped establish the principles of lighter-than-air aircraft and had even been among the first to provide commercial air travel.

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Powerful launcher called Titan IIIC

On June 18, 1965, the expendable launch system Titan IIIC flew for the first time. Used by the U.S. Air Force and NASA from 1965 to 1982, Titan IIIC was a powerful launcher.

Do you know what an expendable launch system is? These are launch vehicles that can be launched only once. This means that the components are either destroyed during re-entry or are discarded in space after launch.

Also called expendable launch vehicles (ELVS), such systems usually contain several rocket stages. As the vehicle gains altitude and speed, these stages typically are sequentially discarded as and when their fuel is exhausted.

The Titan IIIC was one such ELV. Used majorly by the U.S. Air Force and also by NASA, the rocket consisted of modified liquid-fuel first and second stages with two lateral strap-on solid rockets to enhance boost at lift-off.

Began as an ICBM

The Titan family of launch vehicles started off as a large intercontinental ballistic missile (ICBM) as the U.S. Air Force sought an ICBM that would surpass Atlas in terms of delivery capacity and sophistication. Just like the Atlas and Thor, Titan too evolved into an important family of space launch vehicles.

The development contract for what would become the Titan ICBM was issued in October 1955. It was named Titan as the name referred to any of the children of Uranus (Heaven) and Gaea (Earth) and their descendants in Greek mythology. The first Titan was test-launched on February 6, 1959, but Titan I wasn’t modified for spaceflight.

Modified for Gemini Project

 That first happened with Titan Il, a more powerful version of Titan I. Tested successfully in March 1962, Titan II was declared operational in 1963. Initially modified as the Gemini-Titan II to be the launch vehicle of the crewed Gemini Project, it was then used to place satellites in orbit as well.

When there was a need for rockets that were capable of carrying heavier payloads than those handled by Atlas-Centaur, the Titan III family of launch vehicles were born. The Titan IIIA was a Titan II ICBM with an added third stage called transtage, which used twin Aerojet engines and burned Aerozine 50 and nitrogen tetroxide liquid fuel.

Two strap-on boosters

Titan IIIC was an upgrade on Titan IIIA. The most important modification was the addition of two huge strap-on solid rocket boosters that were over 25m tall and 3m wide. They were capable of remarkable thrust as they were powered by burning aluminum/ammonium perchlorate solid fuel.

On June 18, 1965, the Titan IIIC was launched for the first time from Cape Canaveral, Florida with a payload of nearly 10,000 kg. From 1965 to 1982, the Air Force employed different Titan IIICs over 30 times successfully, placing a variety of military communications and reconnaissance satellites in orbit.

In all, there were only five complete or partial launch failures with Titan IIICs. It was also used successfully by NASA for a number of launches, including in 1973 to launch an Applications Technology Satellite.

As long as it was in use, the Titan IIIC was the most powerful launcher that was used by the Air Force. It remained that way until 1982, when Titan 34D, which was based on Titan IIIC, was introduced. The last flight of a Titan IIIC took place on March 6, 1982.

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What about space dust as Earth’s sun shield?

The heat and energy from the sun is what drives life on Earth. That said, humanity is now collectively responsible for so much greenhouse gases that Earth's atmosphere now traps more and more of the sun's energy. This has led to a steady increase in the planet's temperature, and global warming and climate change are causes for concern.

One suggested strategy to reverse this trend is to try and intercept a small fraction of sunlight before it reaches Earth. Scientists, for decades, have considered the possibility of using screens, objects or dust particles to block 1-2% of the sun's radiation and thus mitigate the effects of global warming.

Dust to block sunlight

A study led by the University of Utah explored the idea of using dust to block a bit of sunlight. Different properties of dust particles, quantities of dust and the orbits that would work best for shading Earth were studied. The results were published on February 8, 2023 in the journal PLOS Climate.

Launching dust from Earth to a station at the Lagrange Point between Earth and the sun (L1) would prove to be most effective. The prohibitive costs and efforts involved here, however, might necessitate an alternative, which is to launch lunar dust from the moon.

These two scenarios were arrived at after studying a shield's overall effectiveness, which depends on its ability to sustain an orbit that casts a shadow on Earth. In computer simulations, a space platform was placed at the L1 Lagrange Point (point between Earth and the sun where gravitational forces are balanced) and test particles were shot along the L1 orbit.

While a precise launch was able to create an effective shield for a while, the dust would be blown off by solar winds, radiation, and gravity within the solar system. This would mean that such a system would require an endless supply of dust to blast from L1, making the cost and effort involved astronomical.

Moondust might work

 The second scenario of shooting moondust towards the sun might prove to be more realistic as the inherent properties of lunar dust allow it to work as a sun shield. After studying simulations of lunar dust scattered along different courses, an ideal trajectory that aimed towards L1 was realised.

The authors were clear in stating that their study only looks at the possible impact of such a strategy and do not evaluate the logical feasibility of these methods. If it works, this could be an option in the fight against climate change as it would allow us to buy more time.

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Unsung pioneers in the field of science

These are tales not just of perseverance and love for science, but also of discrimination and unfair treatment. Despite making groundbreaking discoveries, their names remain largely unknown, simply because they are women. Let's celebrate these women scientists and their contribution to the world….

ESTHER MIRIAM ZIMMER LEDERBERG (1922-2006)

Esther Miriam Zimmer Lederberg was an American microbiologist, who discovered bacterial virus Lambda phage and the bacterial fertility factor F (F plasmid). Like many woman scientists of her time, Esther Lederberg was not given credit for her scientific contribution because of her gender. While her husband, her mentor and another research partner won 1958 Nobel Prize in Physiology or Medicine for discovering how genetic material is transferred between bacteria, Esther wasn't even mentioned in the citation, even though her work significantly contributed to the discovery.

Esther Miriam Lederberg was born in Bronx, New York, into a humble family. When studying masters in genetics at Stanford University, Esther struggled to make ends meet. As recollected by Esther in her interviews, she had sometimes eaten frogs’ legs leftover from laboratory dissections.

Esther met her future husband Joshua Lederberg at Stanford. They moved to the University of Wisconsin, where they would begin years of collaboration. Throughout the 1950s, they published papers together and apart, as both made discoveries about bacteria and genetics of bacteria.

Esther Lederberg's contributions to the field of microbiology were enormous. In 1950, she discovered the lambda phage, a type of bacterial virus, which replicates inside the DNA of bacteria. She developed an important technique known as replica plating, still used in microbiology labs all over the world. Along with her husband and other team members, she discovered the bacterial fertility factor.

CECILIA PAYNE-GAPOSCHKIN (1900-1979)

Cecilia Payne-Gaposchkin was a British-born American astronomer who was the first to propose that stars are made of hydrogen and helium.

Cecilia Payne was born in 1900 in Buckinghamshire, England. In 1919, she got a scholarship to study at Newnham College, Cambridge University, where she initially studied botany, physics, and chemistry. Inspired by Arthur Eddington, an English astronomer, she dropped out to study astronomy.

Studying astronomy at Cambridge in the 1920s was a lonely prospect for a woman. Cecilia sat alone, as she was not allowed to occupy the same rows of seats as her male classmates. The ordeal did not end there. Because of her gender, Cecilia was not awarded a degree, despite fulfilling the requirements in 1923. (Cambridge did not grant degrees to women until 1948.)

Finding no future for a woman scientist in England, she headed to the United States, where she received a fellowship to study at Haward Observatory. In her PhD thesis, published as Stellar Atmospheres in 1925, Cecilia showed for the first time how to read the surface temperature of any star from its spectrum. She also proposed that stars are composed mostly of hydrogen and helium. In 1925, she became the first person to earn a PhD in astronomy. But she received the doctorate from Radcliffe College, since Harvard did not grant doctoral degrees to women then. She also became the first female professor in her faculty at Harvard in 1956.

Cecilia contributed widely to the physical understanding of the stars and was honoured with awards later in her lifetime.

CHIEN-SHIUNG WU (1912-1997)

Chien-Shiung Wu is a Chinese-American physicist who is known for the Wu Experiment that she carried out to disprove a quantum mechanics concept called the Law of Parity Conservation. But the Nobel Committee failed to recognise her contribution, when theoretical physicists Tsung-Dao Lee and Chen Ning Yang, who had worked on the project, were awarded the Prize in 1957.

Chien-Shiung Wu was born in a small town in Jiangsu province, China, in 1912. She studied physics at a university in Shanghai and went on to complete PhD from the University of California, Berkeley in 1940.

In 1944, during WWII, she joined the Manhattan Project at Columbia University, focussing on radiation detectors. After the war, Wu began investigating beta decay and made the first confirmation of Enrico Fermi's theory of beta decay. Her book "Beta Decay," published in 1965, is still a standard reference for nuclear physicists.

In 1956, theoretical physicists Tsung Dao Lee and Chen Ning Yang approached Wu to devise an experiment to disprove the Law of Parity Conservation, according to which two physical systems, such as two atoms, are mirror images that behave in identical ways. Using cobalt-60, a radioactive form of the cobalt metal, Wu's experiment successfully disproved the law.

In 1958, her research helped answer important biological questions about blood and sickle cell anaemia. She is fondly remembered as the "First Lady of Physics", the "Chinese Madame Curie" and the "Queen of Nuclear Research”.

LISE MEITNER (1878-1968)

Lise Meitner was an Austrian-Swedish physicist, who was part of a team that discovered nuclear fission. But she was overlooked for the Nobel Prize and instead her research partner Otto Hahn was awarded for the discovery.

Lise Meitner was born on November 7, 1878, in Vienna. Austria had restrictions on women education, but Meitner managed to receive private tutoring in physics. She went on to receive her doctorate at the University of Vienna. Meitner later worked with Otto Hahn for around 30 years, during which time they discovered several isotopes including protactinium-231, studied nuclear isomerism and beta decay. In the 1930s, the duo was joined by Fritz Strassmann, and the team investigated the products of neutron bombardment of uranium.

In 1938, as Germany annexed Austria, Meitner, a Jew, fled to Sweden. She suggested that Hahn and Strassmann perform further tests on a uranium product, which later turned out to be barium. Meitner and her nephew Otto Frisch explained the physical characteristics of this reaction and proposed the term 'fission' to refer to the process when an atom separates and creates energy. Meitner was offered a chance to work on the Manhattan Project to develop an atomic bomb. However, she turned down the offer.

JANAKI AMMAL (1897-1984)

Janaki Ammal was an Indian botanist, who has a flower- the pink-white Magnolia Kobus Janaki Ammal named after her.

She undertook an extraordinary journey from a small town in Kerala to the John Innes Horticultural Institute at London. She was born in Thalassery, Kerala, in 1897.

Her family encouraged her to engage in intellectual pursuit from a very young age. She graduated in Botany in Madras in 1921 and went to Michigan as the first Oriental Barbour Fellow where she obtained her DSc in 1931. She did face gender and caste discrimination in India, but found recognition for her work outside the country.

After a stint at the John Innes Horticultural Institute at London, she was invited to work at the Royal Horticulture Society at Wisley, close to the famous Kew Gardens. In 1945, she co-authored The Chromosome Atlas of Cultivated Plants with biologist CD Darlington. Her major contribution came about at the Sugarcane Breeding Station at Coimbatore, Tamil Nadu. Janaki's work helped in the discovery of hybrid varieties of high-yielding sugarcane. She also produced many hybrid eggplants (brinjal). She was awarded Padma Shri in 1977.

GERTY CORI (1896-1957)

Gerty Cori was an Austrian-American biochemist, known for her discovery of how the human body stores and utilises energy. In 1947, she became the first woman to be awarded the Nobel Prize in Physiology or Medicine and the third woman to win a Nobel.

Gerty Theresa Cori was born in Prague in 1896. She received the Doctorate in Medicine from the German University of Prague in 1920 and got married to Carl Cori the same year.

Immigrating to the United States in 1922, the husband-wife duo joined the staff of the Institute for the Study of Malignant Disease, Bualo. N.Y. Working together on glucose metabolism in 1929, they discovered the 'Cori Cycle' the pathway of conversion of glycogen (stored form of sugar) to glucose (usable form of sugar). In 1936, they discovered the enzyme Phosphorylase, which breaks down muscle glycogen, and identified glucose 1-phosphate (or Cori ester) as the first intermediate in the reaction.

The Coris were consistently interested in the mechanism of action of hormones and they carried out several studies on the pituitary gland. In 1947, Gerty Cori, Carl Cori and Argentine physiologist Bernardo Houssay received the Nobel Prize in 1947 for their discovery of the course of the catalytic conversion of glycogen.

Although the Coris were equals in the lab, they were not treated as equals. Gerty faced gender discrimination throughout her career. Few institutions hired Gerty despite her accomplishments, and those that did hire, did not give her equal status or pay.

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What is the History of science fiction?

Science fiction (sci-fi) has taken us on incredible journeys through time and space, allowing us to explore the depths of our imagination and the limits of the universe.

The term science fiction was first used by William Wilson in 1851 in a book of poetry titled ‘A Little Earnest Book Upon a Great Old subject’. However, the term's modern usage is credited to Hugo Gernsback, who founded the first sci-fi magazine, ‘Amazing Stories’ in 1926. The American editor used this term to describe stories that combined scientific speculation with adventure and futuristic concepts. The term gained widespread use in the 1930s and 1940s and has since become a popular genre of literature and entertainment.

Generally, the beginning of the literary genre of sci-fi is traced to 19th Century England and the Industrial Revolution, a time when rapid technological change inspired and led to the popularisation of stories and narratives that were ideally set in the future and explored themes such as time travel and interplanetary voyages. These stories dealt with the limits of human knowledge and the unintended consequences of our technological prowess. However, literary scholars claim that the earliest literary work that could fit into the genre of sci-fi dates back to the second Century AD.

A True Story: The earliest surviving work of sci-fi

Written by a Syrian satirist Lucian, ‘A True Story’, (also known as ‘True History’) is a two-book parodic adventure story and a travelogue about outer space exploration, extraterrestrial lifeforms, and interplanetary warfare. It is just extraordinary to know that the author produced a story that so accurately incorporated multiple hallmarks of what we generally associate with modern sci-fi, centuries before the invention of instruments such as the telescope.

Lucian was from Samosata (present-day Turkey), and his first language is believed to be Aramaic but he wrote in Greek. He might not be a household name today but literary scholars call him one of antiquity's most brilliant satirists and inventive wits. He is famous throughout European history for producing his absurd yet fantastical works and for his overt dispelling of the ridiculous and ill-logical social conventions and superstitions of his time. His works have been an inspiration for literary classics such as Jonathan Swift's ‘Gulliver's Travels’ and Thomas ‘More's Utopia’.

The basic classification of sci-fi

Sci-fi can be broadly classified into two categories: soft sci-fi and hard sci-fi.

Soft sci-fi, also known as social sci-fi, emphasises the social and humanistic aspects of science and technology, often exploring the effects of scientific advances on society and individuals. Examples of soft sci-fi include Margaret Atwood's The Handmaid's Tale which explores the social and political consequences of a future where women's rights have been severely restricted. Hard sci-fi, also known as scientific or realistic sci-fi, places a greater emphasis on scientific accuracy and realism, often using established scientific principles and theories to explore the possibilities of the future. An example of this is Andy Weir’s ‘The Martian’, which narrates the story of an astronaut stranded on Mars and his efforts to survive by using his scientific knowledge and problem-solving skills.

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What is the role of ISRO in space technology?

The ISRO works to develop and apply space technology in various sectors of our economy.

The Indian Space Research Organisation (ISRO) and the Indian Navy continue to conduct important trials for the Gaganyaan mission. However, do you know what ISRO is?

Organisation

 The ISRO is India's space agency that was established on August 15, 1969.

Previously known as the Indian National Committee for Space Research (INCOSPAR), it was envisioned by Vikram Sarabhai, who helped develop nuclear power in India and is considered one of the founding fathers of Indian space programme. ISRO is a major constituent of the Department of Space (DOS), Government of India.

The department executes the Indian Space Programme primarily through various centres or units within the ISRO.

Works

The ISRO works to develop and apply space technology in various sectors of our economy. It has established major space systems for communication, television broadcasting, and meteorological services.

ISRO's first satellite, Aryabhata, was launched by the Soviet Union on April 19, 1975. Meanwhile, Rohini, the first satellite to be placed in orbit by an Indian-made launch vehicle, was launched on July 18, 1980. It has developed satellite launch vehicles, PSLV (Polar Satellite Launch Vehicle) and GSLV (Geosynchronous Satellite Launch Vehicle), to place the satellites in the required orbits.

These rockets have launched communications satellites and Earth-observation satellites as well as missions to the Moon and Mars – Chandrayaan-1, 2008; Chandrayaan-2, 2019; and Mars Orbiter Mission (MOM), also called Mangalyaan, 2013.

ISRO has launched several space systems, including the Indian National Satellite (INSAT) system for telecommunication, television broadcasting, meteorology, and disaster warning and the Indian Remote Sensing (IRS) satellites for resource monitoring and management. The first INSAT and IRS satellites were launched in 1988.

While ISRO's headquarters is in Bengaluru, the launch vehicles are built at the Vikram Sarabhai Space Centre (VSSC), Thiruvananthapuram. Launches take place at the Satish Dhawan Space Centre on Sriharikota Island, near Chennai.

ISRO's chief executive is a chairman, who is also chairman of the Indian government's Space Commission and the secretary of the Department of Space. Its current Chairman is S. Somnath.

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A test flight with a number of firsts

The 1960s were a rather exciting time if you were part of NASA. After U.S. President John F. Kennedy stated his goal of landing humans on the moon and returning them safely home before the end of the decade of the 1960s, work at NASA progressed at breakneck speed given the enormity of the task ahead of them.

There were a lot of successes along the way, and setbacks too that proved to be equally important in terms of the overall learning. The Apollo-Saturn (AS) 201 mission in the mid 1960s was one such test flight that had a number of firsts, but also experienced malfunctions.

"All-up" philosophy

Coming at the height of Project Gemini, the AS-201 served as a crucial milestone in our march towards the moon. It used the "all-up" philosophy, according to which all components of a system were tested in a single first flight.

A suborbital test flight, its goals included demonstrating the Saturn IB's capabilities, the operation of Apollo Service Module's (SM) main engine, and determining the effectiveness of the Command Module's (CM) heat shield. The Saturn IB rocket, which was built on the 10 successful launches of Saturn 1 rocket, was the most powerful rocket up to that time.

Construction of the AS-201 spacecraft began in 1963 at the North American Aviation (NAA) plant in California. Assembly for the mission began in 1965 with the Saturn IB first stage arriving at the Cape Kennedy Air Force Station (CKAFS), now the Cape Canaveral Space Force Station, on August 14.

Extensively tested

The CM and SM of the spacecraft arrived within two days of each other in October. After successful mating of the two modules and extensive testing, they were trucked to the launch pad and stacked on top of the rocket by December. By January 1966, the final pieces were in place, and the rocket and spacecraft were declared ready for its mission after a flight readiness review and a countdown demonstration.

On February 26, 1966, the AS-201 mission lifted off after a number of launch delays. With flight director Glynn S. Lunney at the helm, a team of engineers kept an eye on all aspects of the mission.

Both stages of the Saturn IB rocket performed well and the Apollo Command and Service Module (CSM) was placed in its suborbital trajectory, with a peak altitude of 488 km. A camera mounted inside the first stage was later recovered at sea, and it had captured some key moments, including the fiery stage separation.

Helium ingestion in propellant lines, however, resulted in lower thrust than predicted during the first burn and the same problem also affected a second burn to test the engine's restart capability. The Service Propulsion System engine also underperformed, meaning the CM entered the atmosphere at a velocity slower than that planned.

Additionally, the capsule rolled during reentry as an electrical fault in the CM led to a loss of steering. The heat shield performed its duties without any flaws despite all these setbacks and the spacecraft splashed down in the Atlantic Ocean, 75 km from the intended target.

On museum display

The largely successful 37-minute test flight travelled 8,472 km overall. The CM was retrieved by swimmers from the prime recovery ship and it was then sent to the NAA plant for postflight inspections. After using it for land impact tests, NASA donated the capsule, which is now on loan and is displayed at the Strategic Air Command and Aerospace Museum.

The Saturn IB is now largely forgotten as its efforts pale in comparison with the Saturn V rocket, one of the largest and most powerful rockets built and which successfully sent people to the moon. But the Saturn IB rocket and the AS-201 mission were all part of the small stepping stones that made the giant leap possible.

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Who was Maria Mitchell?

The astronomer is best known for her discovery of a comet, which later came to be known as ‘Miss Mitchell’s Comet.

Maria Mitchell was the first professional female astronomer in the United States. She is best known for her discovery of a comet, which later came to be known as ‘Miss Mitchell’s Comet

Maria Mitchell was born in 1818 in Nantucket, Massachusetts. Her father was a school principal and an amateur astronomer who helped her develop interest in science and astronomy at an early age. Maria would spend hours observing the night sky through a telescope and help her father in such calculations as predicting annual eclipses. Through her jobs as a teacher and later as a librarian, Maria Mitchell kept her passion for astronomy alive. Her success in establishing the orbit of a new comet in 1847 gained her international repute. She received a gold medal from the King of Denmark for this discovery.

Later, she took up a job as professor of astronomy at Vassar College in New York. Mitchell and her students continuously tracked and photographed sunspots. She was the first to find that sunspots were whirling vertical cavities and not clouds, as had been earlier believed. In 1882, she documented Venus traversing the sun-one of the rarest planetary alignments known to man.

Maria Mitchell was also a well-known proponent of equal rights-she fought relentlessly for women as well as for blacks. The school that she started admitted black children at a time when segregation was common in the US. At Vassar College, she demanded and got equal pay when she realised that her junior male colleagues were paid more.

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When was the third human landing on the moon?

On February 5, 1971, Apollo 14 made a successful landing on the lunar surface, thereby becoming the third human landing on the moon after Apollo 11 and Apollo 12.

When we talk about the Apollo programme, it is often hard to look beyond the Apollo 11 mission, which achieved the distinction of landing the first humans on the moon. Even though the Apollo programme is best remembered for this, it should also be noted that it provided for innumerable demonstrations of ingenuity and problem solving and increased NASA’s expertise by leaps and bounds.

Following the success of Apollo 11 in July 1969, Apollo 12 landed humans on the moon in November 1969. Apollo 13, however, had to be aborted following an oxygen tank explosion in the service module.

This meant that the Fra Mauro Formation, originally planned to be the lunar landing site for Apollo 13, served as the landing site for Apollo 14, once NASA had completed an accident investigation and upgraded the spacecraft.

Shepard, Mitchell, and Roosa

Launched on January 31, 1971, Apollo 14 had a three-member crew that included commander Alan Shepard, lunar module pilot Edgar Mitchell, and command module pilot Stuart Rossa. Even though there was a potential short circuit in an abort switch on the lunar module and the landing radar came on very late during the landing sequence, Shepard and Mitchell successfully landed on the lunar surface on February 5. In fact, it was the most precise landing until then, as they landed less than 100 feet from the targeted point.

Shepard and Mitchell spent over 33 hours on the moon, including two extra vehicular activities (EVAS) that spanned nine hours and 23 minutes. Even though the first of the two EVAS began an hour later than scheduled due to communications systems problems, it turned out to be a success.

Modular Equipment Transporter

The first EVA was mainly to deploy a number of experiments and some of these sent back data to Earth until September 1977. While a seismometer detected thousands of moonquakes and helped find out the moon’s internal structure, other instruments looked at the composition of solar wind and the moon’s atmosphere.

Apart from the safety upgrades that were done for Apollo 14, there was also the addition of the Modular Equipment Transporter (MET). While Apollo 11 astronauts carried their tools by hand and Apollo 12 astronauts used a hand tool carrier, Shepard and Mitchell could employ the MET like a wheelbarrow, stowing away their scientific equipment, tools, camera, and sample collections.

During the duo’s second EVA dedicated to explore the Cone Crater, the MET came in handy as they were able to pick up a football-sized rock, designated 14321, but better known by its nickname “Big Bertha”. Using the MET, the astronauts were able to transport this sample back to the lunar module. As recently as 2019, studies suggested that a two-cm sliver of the Big Bertha might have originally come from the Earth’s crust, and not the moon.

42 kg of samples

Even though the crew never saw the interior of the crater, post-mission comparisons showed that Shepard and Mitchell were within 50-75 m from the crater rim. The round trip lasted four hours and 35 minutes in which the duo traversed nearly 3 km, including samples from the first EVA, the duo had collected 42 kg of lunar samples.

While Shepard and Mitchell were busy on the lunar surface, Roosa, who was in the command module, clicked many pictures in high resolution. These photographs of the moon’s Descartes region played a pivotal role in certifying the area’s safety as a landing site and even helped plan rover traverses for the Apollo 16 mission.

Liftoff from the lunar surface took place exactly on schedule, while rendezvous and docking with the command module was just two minutes off schedule. After spending 2.8 days in lunar orbit, during which time the command module had circled the moon 34 times, the Apollo 14 crew members headed back to Earth. They splashed down safely in the Pacific Ocean on February 9, exactly nine days and two minutes after launch.

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What was the Mercury space capsule project?

On June 11, 1963, the Mercury space capsule was patented and assigned to NASA. The patent was received less than a month after the last flight of Project Mercury had been carried out.

Receiving a patent generally signals a major milestone. As an exclusive right granted for an invention, be it a product or a process, it usually denotes a new way of doing something, thereby becoming important. In the case of the Mercury space capsule, however, the patent came closer to the end.

Project Mercury was conceived as a NASA programme to put the first American astronauts in space. Named after a Roman god who was very fast, the project notched up many successes. At the centre of this success was the Mercury space capsule.

“Space capsule”

The principal designer of the Mercury spacecraft was Maxime Faget, a mechanical engineer who also contributed to the designs of the Gemini and Apollo spacecraft. Faget, along with Andre Meyer, Robert Chilton, Willard Blanchard Jr., Alan Kehlet, Jerome Hammack and Caldwell Johnson filed for a patent titled “Space capsule” on October 16, 1959.

In this patent application, they described their invention relating to space vehicles as a “manned capsule configuration capable of being launched into orbital flight and returned to the Earth’s surface.”

Additionally, it was capable of providing “protection for its occupant from the deleterious effects of large pressure differentials, high temperatures, micrometeorite collisions, high level acoustical noise, and severe inertial and impact loads.”

Not cosy

It did all that, but the capsule was a rather small one, with room for just one astronaut. What’s more, this astronaut had to stay seated throughout the flight. While there was very little room for even the single seated astronaut to make any movements, it was argued that not much was required as the pilot would only need to move his arms and head, and was to never leave the spacecraft during flight.

Following uncrewed flights and those with primates as part of Project Mercury, the first crewed flight took place on May 5, 1961. Alan Shepard made the first crewed Mercury flight in a capsule that he named Freedom 7. The 15-minute flight that went into space and came back down made him the first American in space.

Between 1961 and 1963, there were six successful flights as part of Project Mercury that showed that Americans could fly in space. While two of these flights were suborbital flights (reached space and came right back down), the other four made it into orbit and circled our Earth.

Every time the Mercury spacecraft re-entered the Earth’s atmosphere, the blunt end came in first to not only slow down the spacecraft, but also shed the heat caused by friction with the air during the descent. With layers of heat resistant ablative resins coating the curved heat shield, it charred away to minimise structural heating, preventing damage to the spacecraft, and of course, protecting the crewman.

The last of the six successful crewed Mercury Project spaceflight took place on May 15, 1963. Each of these flights lasted from 15 minutes to 34 hours, with most lasting less than nine hours.

Just a formality

This meant that by the time the patent for the Mercury capsule was awarded on June 11, 1963, it had already been put to use multiple times successfully, with each of the successes celebrated by an entire country. The patent, which was assigned to NASA, was merely a formality.

In fact, NASA retired the Mercury capsule in the same week in which the patent was awarded. The first manned space vehicle of the U.S. was retired with honours of course, having been central to a project that came at the height of the space race between the U.S. and the Soviet Union.

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When was the last human expedition to the moon?

On December 11, 1972, Apollo 17 achieved lunar landing. The sixth mission in the Apollo program to explore the lunar surface, Apollo 17, for now, is the last human expedition to the moon.

Apollo 11 will forever be remembered as the mission which enabled human beings to set foot on the moon, our natural satellite, for the first time. While the first will always remain the the same cannot be said for what is the last such mission, as future missions might take that place. But for the time being, Apollo 17 remains the last human expedition to the moon.

After the success of Apollo 11 in 1969, there were six more Apollo missions to the moon, five of which were successful. As U.S. President John F. Kennedy’s objective of landing humans on the moon had been achieved, NASA faced funding cuts. Technology and research-based missions weren’t seen as important as the landing itself, forcing NASA to cancel some of the planned missions in 1970. As a result, the Apollo 17 mission of 1972 became the last manned mission to the moon.

Firsts and records

Apollo 17 was a 12-day mission that spanned from December 7-19. Apart from the distinction of being the last human expedition to the moon for now, Apollo 17 also achieved a number of firsts and broke some records. It had the then longest space walk and enabled the collection of the largest lunar samples brought back to Earth. It was the first Apollo mission to be launched at night and allowed a scientist to walk on the moon for the first time.

The scientist in question was Harrison H. Schmitt, a geologist who had been part of the backup crew for Apollo 15. Schmitt was originally scheduled to go on Apollo 18, which was cancelled. The scientific community lobbied for Schmitt’s inclusion in Apollo 17. While Schmitt served as the pilot of the lunar module “Challenger”, Eugene A. Cernan was commander and Ronald E. Evans was the pilot of “America”, the command module.

Following a successful night launch on 7, Apollo 17 achieved lunar orbit insertion on December 10. Then, with Evans orbiting the moon, Cernan and Schmitt flew Challenger and landed on the moon’s surface on December 11, touching down within 200 m of the targeted landing point.

Two primary objectives

Apollo 17’s two primary objectives were to obtain a specific sample and to explore geologically recent, explosive volcanism. The former was achieved as they retrieved the oldest known unshocked (unaltered by meteoric impact) rock from the moon. This sample, called Troctolite 76535, is believed to be at least 4.2 billion years old.

The second objective was met as Schmitt discovered orange soil near Shorty crater. This colour was the result of orange and black volcanic glass that had formed in the type of volcanic eruption that is referred to as “fire fountain” on Earth.

Cernan and Schmitt were on the lunar surface for 75 hours, the longest till now. They clocked 22 hours of extravehicular activity (EVA) with the help of their rover and travelled about 36 km. They went as far as 7.4 km away from the Challenger, close to the limit of what was considered the walk-back distance possible, should the rover have failed. Apart from conducting various experiments, they took over 2,000 photographs and collected 110 kg worth of soil and rock samples from 22 different sites.

Last man on the moon

Following the third and final EVA, the duo televised the unveiling of a plaque with a message, which they left on the moon. On December 14, Cernan took humankind’s final step, to date, off the moon.

After lifting off from the moon, the Challenger was docked with America on December 15. Four days later, on December 19, the Apollo 17 capsule splashed down in the Pacific Ocean at a distance of 6.5 km from the recovery ship, after a mission elapsed time of 301 hours.

For 50 years, Cernan has often been referred to as the last man on the moon. With NASA’s Artemis program aiming to return to the moon and even set up a sustained human presence, it might not be long before the next human being sets foot on the moon.

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Which is the smallest planet in the solar system?

Mercury is the smallest planet in our solar system. Located closest to the Sun, it is also the fastest planet in our solar system, travelling at a speed of nearly 47 kilometres per second. In fact, the closer a planet is to the Sun, the faster it travels. Mercury completes one circle around the Sun in just about 88 Earth-days.

When observed from its surface, the Sun would appear more than three times as large as it does when viewed from Earth, and the sunlight is as much as seven times brighter. But despite this proximity to the Sun, Mercury is not the hottest planet in our solar system- it is Venus. The reason for this is Venus’ dense atmosphere.

Another interesting aspect of Mercury is that the Sun appears to rise briefly, set, and rise again from some parts of the planet’s surface due to its elliptical and egg-shaped orbit, and sluggish rotation. The same phenomenon happens in reverse during sunset.

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What is Protogalaxy?

A protogalaxy is in simpler words a primeval galaxy. It refers to a galaxy that is undergoing the first generation of star formation. It is also defined as a cloud of gas that is forming into a galaxy. This particular celestial mass would just comprise hydrogen gas trapped in some dark matter prior to the initial stages of star formation. The stars are formed from the smaller clumps of gas in the protogalaxy.

Types of Galaxies

There are two types of galaxies viz. elliptical galaxies and spiral galaxies. The majority of the galaxies that you come across are elliptical galaxies and they are called so because they have an even, ellipsoidal shape. They also are comprised with a greater population of older stars when compared to spiral galaxies.

A spiral galaxy normally has a rotating disc replete with spiral ‘arms. The stellar orbits are circular in shape and they have a flattened disk system. Most spiral galaxies also contain in their centre a mini-elliptical galaxy. Our galaxy, the Milky Way, is a spiral galaxy.

So what determines the shape of a galaxy? The rate of star formation during galactic evolution determines whether it turns out into a spiral or elliptical galaxy. If the star formation is at a slower pace, then it turns into a spiral galaxy.

Milky Way

About 12.5 billion years ago, the Milky Way started to form. Several huge clusters of stars and clumps of gas fused together to form a protogalaxy. This was the building basis of our home!

It then collided with many galaxies, and after a lot of mergers, it acquired its present form.

Recently, scientists discovered a population of millions of stars at the center of our galaxy. Those were the remains of the ancient protogalaxy! These oldest stars that were found in the core area of our galaxy were analysed and the scientists found out that they were part of a protogalaxy.

The diameter of which extended to 18 thousand light-years, and with a mass that was 50-200 million times that of the Sun!

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Why are astronomers concerned about light pollution?

Light pollution is very much a concern across the globe, something astronomers and skywatchers are trying to bring attention to. It not only takes away the right to enjoy the night skies and explore the celestial bodies with the naked eye but also affects the circadian rhythm of humans and wildlife.

Have you seen a sky spangled with stars winking at you from light years away? Have you ever spotted the Milky Way?

Well with the amount of artificial light strewn across the sky. it is a fact that dark skies that bring out the beauty of the cosmos are a rarity.

Light pollution is very much a concern across the globe, something astronomers and skywatchers are trying to bring attention to. It not only takes away the right to enjoy the night skies and explore the celestial bodies with the naked eye but also affects the circadian rhythm of humans and wildlife. So what is light pollution?

Light Pollution

Across the world, people have to deal with the nighttime glow caused by artificial light. This has been affecting humans, wildlife, and the environment equally. There is a global movement to reclaim the dark sky and reduce light pollution.

Sources of light pollution

The major cause of light pollution is misdirected light which scatters out into the open sky caused by human activities. From street lights to lights from buildings, boats, and outdoor advertising to illuminated sporting venues, every misdirected light leads to light pollution. High levels of sky glow mean fewer chances of seeing enough celestial bodies in the sky.

The circadian rhythm and light pollution

Artificial light can affect the circadian rhythm in both humans and animals. The circadian rhythm is the natural process regulating the sleep-wake cycle. The production of the hormone melatonin is linked to this. This sleep-inducing hormone gets released when it is dark. The presence of light inhibits it. If the ambient light is high at night, then it lowers the production of melatonin and leads to sleep deprivation, stress, fatigue, and anxiety.

Animal behaviour and light pollution

It has been proven that wildlife has also been affected badly by light pollution. The animal behaviours such as migration patterns and wake-sleep habits of animals have been affected. Birds and sea turtles have been found to lose their way and get confused due to the presence of increased ambient light. Light also affects the circadian rhythm of animals.

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What was the Centaur project?

The Centaur upper stage rocket is a family of high-energy rockets that has played a pivotal role in advancing global communications and furthering our knowledge of space. November 27, 1963 is an important day in its history as it marked the first in-flight burn of a liquid hydrogen/ liquid oxygen engine.

When we speak about successful space missions, we generally talk about the results they delivered – the satellites that now orbit the Earth or the probes that gathered invaluable data from other planets. There’s a lot of work and plenty of factors, however, that goes into reaching that point. One of them is the upper stage rocket that boosts satellites into orbit and propels probes into space.

Among upper stage rockets, Centaur is a significant achievement as it has served as America’s workhorse in space and has been involved in many success stories. Used for over 100 unmanned launches, Centaur has expanded the frontiers of space and revolutionised communication.

Where it all began

Centaur’s beginnings predate even the existence of NASA as the U.S. Air Force studied a proposal from General Dynamics/ Astronautics Corp. to develop a new booster stage in 1957. With the space race between the U.S. and the Soviet Union heating up during this period, the idea was to give the country an edge, providing a means of orbiting heavy payloads in a very short time.

In 1958, the year NASA was established, Centaur became an official hardware programme with the Air Force as its assigned development authority. While the heaviest Soviet satellite orbiting the Earth at this time was the 1,360-kg Sputnik III, the U.S. had plans for boosting payloads to up to 3,850 kg. They planned to achieve this using Centaur, which was to have a new propulsion system using liquid hydrogen, mixed with liquid oxygen.

By July 1959, Centaur moved from the jurisdiction of the Department of Defense to NASA. Centaurs planned schedule of testing and operation, however, proved too optimistic, as there were a mountain of problems, failures, and delays to overcome.

Silverstein provides the silver lining

In 1962, American engineer Abe Silverstein put his hand up and convinced NASA that his Lewis Research Center could debug the Centaur and manage its problems. Once the entire responsibility was assigned to Lewis under Silverstein, the Lewis engineers got to work, perfecting the booster, while carrying out complex research and development to ensure Centaurs reliability. The fact that Lewis had been involved in pioneering work on high-energy liquid propellants for rockets helped, as this meant that most engineers working with Centaur were already aware of safely handling the liquid hydrogen/ liquid oxygen cryogenic fuels that it used.

The original Centaur rocket measured 30 feet long and 10 feet in diameter. As it used very cold propellants (liquid oxygen at-297 degrees Fahrenheit and liquid hydrogen at -420 degrees Fahrenheit), its tanks required special construction. A doubled walled bulkhead not only served as a heat barrier, but also separated the two compartments containing liquid hydrogen and liquid oxygen. Made of stainless steel less than 200ths of an inch thick, the tank was extremely thin and light-weight even once pressurised.

Following successful assembly, inspection, and shipping to Cape Canaveral, engineers and technicians perform testing procedures that can last weeks. A special tiger team uses a checklist to go through it all once again in the days leading up to any launch, before putting the rocket into start condition for the flight.

Go Centaur!

On November 27, 1963, one such launch took place. While it only carried a dummy payload that was put into orbit, it was a significant milestone. This was NASA’s first successful launch of the Atlas Centaur, proving the compatibility of the Atlas rocket with the upper stage Centaur. Additionally, it had the first in-flight burn of a liquid hydrogen/liquid oxygen engine, showing that these could be safely fired in space. In the decades that followed, there were many more successes for Centaur and a few mishaps too. Centaur was involved in sending the unmanned Surveyor spacecraft, which collected data on the moon’s surface and paved the way for the Apollo missions. Along with Atlas and Titan boosters, Centaur featured as the upper for probes and flybys to all other planets in our solar system.

It didn’t stop there as Centaur also launched orbiting observatories that help expand our knowledge about the universe, peering at space beyond our solar system. Centaur was also involved in launching various satellites into geosynchronous orbits that have changed the face of communication on our planet. While its name might not be often mentioned along with successful missions, Centaur continues to be a workhorse that serves its purpose.

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Which is the largest planet?

The largest planet in our solar system, Jupiter, is located fifth from the Sun. It is more than two times the size of all the planets in our solar system combined. Jupiter has also been instrumental in our understanding of the universe and our place in it. In 1610, Galileo discovered Jupiter’s four large moons: lo, Europa, Ganymede and Callisto. This confirmed the Copernican view that the Earth was not the centre of the universe as these newly discovered celestial objects were revolving around another planet.

It is estimated that eleven Earths could fit across Jupiter’s equator. To put it in other words, if our planet is the size of a grape, then Jupiter is the size of a basket-ball. It has an iconic Great Red Spot, which is a giant storm that has been active in Jupiter’s atmosphere for hundreds of years. This storm is bigger than the Earth!

Jupiter’s orbit is about 778 million kilometres or 5.2 Astronomical Units (AU) from the Sun (Earth is one AU from the Sun). Jupiter is a gas giant, which lacks an Earth-like atmosphere. Even if it has a solid inner core at all, it would only be about the size of the Earth. Jupiter’s atmosphere contains mainly hydrogen (H) and helium (He) and has more than 75 moons. It rotates about its axis once every 10 hours (a Jovian day), and takes about 12 Earth years to complete one revolution about its orbit around the Sun (a Jovian year).

In the year 1979, NASA’s Voyager mission discovered Jupiter’s faint ring system. We have discovered that all the four giant planets of our solar system have ring systems. Till date, nine spacecraft have visited Jupiter. Of them, only the most recent one landed on Jupiter. Seven of them only flew by this gas giant and the other two just orbited it. Juno, the latest spacecraft, arrived on Jupiter in 2016.

Although it is the biggest planet in our solar system, Jupiter cannot support life as we know it. But we have come to know that some of its moons have oceans beneath their crusts, which could possibly support some form of life.

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What are dwarf galaxies?

As their name suggests, dwarf galaxies are smaller galaxies. In contrast to a normal galaxy that comprises hundreds of billions of stars, a dwarf galaxy would contain just about a few billion stars. These dwarf galaxies orbit larger galaxies after their formation.

Formation of dwarf galaxies

The dwarf galaxies are created when two galaxies collide, fromed from the material and dark matter coming out of the galaxies that collided.

Following these collisions, while a significant portion of the gas, dust and stars emitted gets reincorporated into the galaxy created after the collision, some can lead to the formation of dwarf galaxies which then orbit around the galaxy. They are also formed by the gravitational forces existing during the creation of these larger galaxies.

Why are dwarf galaxies crucial

Scientists consider the dwarf galaxies critical as they could help gain insight into the early stages of the formation of galaxies and stars. According to scientists, our galaxy has about 14 satellite dwarf galaxies orbiting it.

Studies are being carried out on these dwarf galaxies as it would give us clues regarding the evolution of the galaxies. By studying the motion of the stars in these galaxies, we would also get to know more about dark matter and how it is distributed in the galaxies.

It is difficult to spot dwarf galaxies as they are less bright when compared to larger galaxies. A large number of them can be spotted in galaxy clusters or as a companion to larger galaxies.

Shapes of dwarf galaxies

The dwarf galaxies take several shapes. The dwarf elliptical galaxies are quite similar to normal elliptical galaxies.

Then there are dwarf spheroidal galaxies which are more spherical in shape and smaller when compared to the former.

Then we have the irregular dwarf galaxies. They do not have a distinct structure and are rich in gas.

One of the closest dwarf galaxies to the Milky Way is the Sagittarius Dwarf Spheroidal Galaxy.

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How did Japan’s Hayabusa spacecraft collect samples from an asteroid?

Scientists study meteorites for clues about the origin of Earth and the solar system because most meteorites are bits of asteroids that have fallen to Earth, and asteroids are believed to be leftover material from the time the solar system formed.

In 2005, for the first time ever, scientists scooped up rock samples directly from an asteroid using a spacecraft built especially for that purpose. The name of the spacecraft was Hayabusa. It was a robotic spacecraft developed by the Japan Space Exploration Agency (JAXA).

Hayabusa (Japanese for falcon’) was launched on May 9, 2003, and arrived in the vicinity of the asteroid Itokawa in mid-September 2005. In November 2005, it landed on the asteroid and collected samples in the form of tiny grains of rock which it brought back to Earth on June 13, 2010. Hayabusa was the first spacecraft to land and take off from an asteroid.

In December 2014, Japan launched another spacecraft Hayabusa 2 to study the near-Earth asteroid Ryugu and to bring back samples of rock not only from its surface but also from deeper below the surface. Hayabusa 2 reached Ryugu in June 2018.

In September 2018, the spacecraft landed two rovers on the asteroid. They were the first rovers ever to move on an asteroid. They moved with a hopping movement instead of rolling around on wheels. The rovers are designed to take pictures of the landscape and measure the temperatures on the asteroid.

Hayabusa 2 left the asteroid in November-December 2019 and delivered a small capsule that contained the rock and dust samples when it was 220,000 km from the Earth’s atmosphere. The capsule safely landed in the South Australian outback in December 2020.

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What are brown dwarfs?

Brown dwarfs are also known as failed stars. Why? Find out

Brown dwarfs are celestial objects that are too large to be called planets and too small to be called stars. They have. a mass less than 0.075 that of the sun, which is around 75 times the mass of Jupiter. Like stars, brown dwarfs are believed to form from a collapsing cloud of gas and dust. But as the cloud collapses, it does not form an object dense enough at its core to trigger a nuclear fusion. In the case of a star, hydrogen is converted into helium by nuclear fusion. This is what fuels a star and causes it to shine. Brown dwarfs, on the other hand, are not massive enough to ignite fusion. Hence, they are also called ‘failed stars’.

Dimmer and cooler than stars, brown dwarfs are elusive and hard to find. Infrared sky surveys and other techniques have, however, helped scientists detect hundreds of them.

They are believed to be as common as stars in the Universe. Some of them are companions to stars and many are isolated objects.

First discovered in 1995, brown dwarfs were hypothesized in 1963 by American astronomer Shiv Kumar. Despite their name, brown dwarfs are not brown. They appear from deep red to magenta, depending on their temperature.

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What are the secrets of Enceladus moon?

Discovered on August 28, 1789, Enceladus is a natural satellite of Saturn. This moon, which remained in relative obscurity for nearly 200 years, is now one of the most scientifically interesting destinations in our solar system.

The possibility of worlds other than our own Earth where life could exist has enthralled us for a long time. Often seen in the realm of science fiction, we might be inching ever so closer to it in reality as scientists have identified a handful of worlds that have some of the ingredients needed for life. One of them is Enceladus, an icy moon that is the brightest in the solar system.

Enceladus was discovered on August 28, 1789 by British astronomer William Herschel, more popular for discovering the planet Uranus. Little is known about how William went about it and made his discovery.

A dwarf named after a giant

What we do know, however, is that it was William’s son, John Herschel, who gave the moon its name Enceladus, after the giant Enceladus of Greek mythology. In his 1847 publication Results of Astronomical Observation made at the Cape of Good Hope, John suggested names for the first seven moons of Saturn that had been discovered, including Enceladus. He picked these particular names as Saturn, known in Greek mythology as Cronus, was the leader of the Titans.

For nearly two centuries, very little was known about Enceladus. That changed in the 1980s, when the U.S. spacecrafts Voyager 1 and Voyager 2 flew by the moon, capturing images. The pictures indicated that the icy surface of this small moon is very smooth in some places and bright white all over.

Enceladus, in fact, is the most reflective body in the solar system. Scientists, however, didn’t know why this was the case for a few more decades. Enceladus reflective capability implies that it reflects almost all the sunlight that strikes it, leading to extremely cold surface temperatures, of the order of -200 degree Celsius.

E ring and tiger stripes

Shortly after NASA’s Cassini spacecraft began studying Saturn’s system in 2004, Enceladus started revealing its secrets. By spending over a decade in the vicinity of the small moon, including flybys as close as 50 km, Cassini was able to unearth a wealth of information about Enceladus.

Cassini discovered that icy water particles and gas gush from the moon’s surface at about 400 metres per second. These continuous eruptions create a halo of fine dust around the moon, which supplies material for Saturn’s E ring. While a small fraction of this remains in the ring, the remaining falls like snow back onto the moon’s surface, thereby making it bright white. Scientists informally call the warm fractures on Enceladus’ crust from which the water jets come from as “tiger stripes”.

By measuring the moon’s slight wobble as it orbits Saturn and from gravity measurements based on the Doppler effect, scientists were able to determine that these jets were being supplied by a global ocean inside the moon. As this ocean supplies the jet, which in turn produces Saturn’s E ring, it follows that studying material from the E ring is akin to studying Enceladus’ ocean.

While the E ring is mostly made of ice droplets, there is also the presence of nanograins of silica that can be generated only where liquid water and rock interact at temperatures above 90 degrees Celsius. Along with other evidence that has been gathered, this suggests the existence of hydrothermal vents deep beneath this moon’s shell, similar to those on the Earth’s ocean floor.

Orbital resonance

Enceladus takes 33 hours for its trip around Saturn, which is nearly half of the time taken by the more distant moon Dione. Enceladus is thus trapped in an orbital resonance with Dione, whose gravity stretches Enceladus’ orbit into an elliptical shape. This means that Enceladus is sometimes closer to Saturn and at other times farther leading to tidal heating within the moon.

Running just over 500 km across, Enceladus is small enough to fit within the Indian State of Maharashtra, which runs around 700 km north-south and 800 km east-west. What it lacks in size it more than makes up for in stature, as Enceladus has a global ocean, unique chemistry, and internal heat. All this means that even though we still have plenty of data about the moon to pore over, explorers will eventually plan a return to Enceladus to learn more of its secrets.

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Who is the first Latin American to fly into space?

Arnaldo Tamayo Méndez, (born Jan. 29, 1942, Guantánamo, Cuba), Cuban pilot and cosmonaut, the first Latin American, the first person of African descent, and the first Cuban to fly in space. After the revolution of 1959, Tamayo Méndez joined the Cuban air force as a pilot.

Born in 1942, Mendez makes no mention of his father in his book Un cubano en el cosmos (A Cuban in the cosmos). As he lost his mother to tuberculosis while just eight months old, he grew up as a poor orphan in Guantanamo.

Limited schooling

He worked as a shoeshine boy, sold vegetables, delivered milk and worked as an apprentice carpenter by the time he reached his teenage years. Even though he had limited opportunities for schooling, he excelled at it in whatever little chance he got.

After joining the Association of Young Rebels during the Cuban Revolution, Mendez made his way to a technical institute. Here, he saw a chance to pursue his dream of flying and he readily enrolled himself into a course for aviation technicians, passing it with flying colours in 1961.

His success at this course gave him the confidence to become a pilot and make his dream a reality. He was then selected to travel to the Soviet Union to further his studies and learn to fly the Soviet MiG – 15 fighter jet. Mandez rose through the ranks in the next 15 years, becoming a captain in the Cuban Air Force by 1978.

Interkosmos programme

During the time Mendez was making his way up the Cuban Air Force, the Soviet Union had designed and formed the Interkosmos space programme (1967) and had the first flight of this programme in 1978. The objective of Interkosmos was to help the Soviet Union’s allies with crewed and unscrewed missions to space.

The search for the first Cuban Cosmonaut began in 1976 and a long list of 600 was shortlisted to two by 1978: Mendez and the other being Jose Lopez Falcon. It could have been purely based on merit, or it might have been an act of propaganda with political motivations, but what we do know is that Mendez was selected to fly aboard the Soyuz 38 mission.

On September 18, 1980, Mendez created history as he flew aboard Soyuz 38 along with Soviet cosmonaut Yuri Romanenko. On that same day, they docked at the Salyut 6 space station, and Mendez met Soviet cosmonauts Leonid Popov and Valery Ryumin as the hatch opened and was sealed.

Over the next seven days, Mendez completed 124 orbits around the Earth, conducting a number of experiments on science and health. There were a total of nine experiments, including those that studied stress, blood circulation, immunity, balance, and the growth of a single crystal of sucrose in weightlessness.

Instant fame

Mendez and Romanenko landed back on Earth on September 26 and the former was lauded by both the Cubans and the Soviets Mendez became an instant national hero and was honoured with the Hero of the Republic of Cuba medal, and received The Order of Lenin from the Soviets, among many other recognitions.

Mendez, who is now an 80-year-old, rose to the position of brigadier general following his space flight. He spent many years leading the education efforts of the Cuban army. Cuba’s Museum of the Revolution in Havana is home to the space suit that Mendez used for his historic Voyage.

The Interkosmos programme successfully flew many non-Soviets, including India’s Rakesh Sharma and astronauts from Britain, Japan, France, and Vietnam, among many other countries. Mendez’s flight not only made him the first Cuban cosmonaut, but also the first with African heritage to make it to space.

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What is Avatar?

AVATAR is an acronym for “Aerobic Vehicle for Hypersonic Aerospace Transportation”.

It is a single stage reusable space plane which is capable of horizontal take-off and landing. It is an unmanned spacecraft. DRDO is working on it. This can make satellite launches much cheaper as they can take off from conventional airfields. AVATAR’s liquid air cycle engine collects air on the way up, liquefies it, separates oxygen and stores it on board for flight beyond the atmosphere. AVATAR was first announced in May 1998 at the Aero India 98 exhibition held at Bangalore.

AVATAR was a follow up on the ‘Hyperplane’, a dream project of Dr. Kalam in the 1980s. The Hyperplane projects failed due to their immense weight. AVATAR weighs only 25 tonnes. And 60 per cent of it is liquid hydrogen fuel. It can launch satellites weighing one tonne!

The AVATAR design has been patented in India. Applications for registration of the design have been filed in patent offices in the US, Germany, Russia and China.

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What is small satellite launch vehicle?

The Indian Space Research Organisation has been successful at developing space launch vehicles, building satellites, and launching them. But the space agency faced a glitch recently on the maiden journey of its Small Satellite Launch Vehicle (SSLV). Let’s see what an SSLV is.

As the name suggests, an SSLV is a small satellite launch vehicle capable of launching lightweight satellites. The ISRO’s SSLV is 34 metres tall, weighs 110 tonnes, and is equipped to launch satellites weighing between 10 kg and 500 kg to low earth orbit (LEO), that is up to 500 km from Earth. Such lightweight satellites are also called mini, micro, or nano satellites.

The SSLV has been developed to cater to the emerging market for the launch of small satellites into Earth’s low orbits by developing countries, students, and others. The SSLV is the third offering of the ISRO after the Polar Satellite Launch vehicle (PSV) and the Geosynchronous Satellite Launch Vehicle (GSLV). The key features of the SSLV are low cost, flexibility in accommodating madtiple small satellites, possibility of multiple drop-offs launch-on-demand feasibility, and minimal launch infrastructure requirement On its maiden demonstration flight on

August 7, the SSLV carried an earth observation satellite (LOS-02), and a cube satellite developed by students, named AzandiSAY. The rocket was supposed to place the payloads into the desired 356 km circular orbit. But the satellites were instead placed in an elliptical orbit. It was said the rocket deviated from its path and placed the satellites into 356/76 km low earth orbit due to malfunctioning of a sensor. “As the 76 km elliptical orbit was the lowermost point and closer to the surface of the Earth the satellites placed in such an orbit will not stay for long due to the atmosphere and will come down. The (two satellites) have already come down from that orbit and are no longer usable according to ISRO Chairman S. Somanath.

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Why did the Mars Observer fail?

On August 22, 1993, just days before the Mars Observer spacecraft was to enter orbit around Mars, it lost contact with the bases here on Earth. The $400 million spacecraft with an estimated overall project cost of $1 billion was designed to study and photograph the Martian surface, but ended in failure.

Following the success of the Mariner programme in the 1960s and early 70s, the Viking programme was the U.S.’s next foray towards our neighbouring planet, Mars. After the probes Viking 1 and Viking 2 successfully landed on the red planet in 1976, over a decade went by before America’s next mission to Mars. That came in the way of the Mars Observer, which was launched in 1992 and had things going well until its ill-fated end.

The mid-1980s saw a high priority mission to Mars being planned to act and expand on the information already assimilated by the Viking programme. With the preliminary mission goals of studying and taking high-resolution photographs of the Martian surface, the Mars Observer spacecraft was initially to be launched in 1990, before being rescheduled to 1992.

Based on Earth-orbiting spacecraft

Based on a commercial Earth-orbiting communications satellite that had been converted into an orbiter for Mars, the spacecraft was built at a cost of $400 million. The payload was made up of a variety of instruments that included a Gamma Ray Spectrometer (GRS), Pressure Modulator Infrared Radiometer (PMIRR), Thermal Emissions Spectrometer (TES), Mars Observer Camera (MOC), and Mars Balloon Relay (MBR) among others.

The specific objectives of the mission were to find out the elemental characteristics of the Martian surface: defining Mars topography and gravitational field: establishing the nature of Mars magnetic field finding out the distribution and sources of dust and volatile material over a seasonal cycle: and exploring the Martian abmosphere. The MBR was designed to receive information from the planned Mars Balloon Experiment to be carried by a Russian mission for retransmission back to Earth.

Contact lost

The Mars Observer was expected to achieve all this by orbiting the planet for one Martian year (687 Earth days), giving it a chance to observe the planet through the different seasons. The science instruments in the payload were thus designed to study the geology, climate, and geophysics of Mars.

Following a successful launch on September 25, 1992, Mars Observer was scheduled to perform an orbital insertion manoeuvre 11 months later on August 24, 1993. Just days before it, however, on August 22, 1993, communication was lost with the spacecraft even as it was preparing to enter orbit.

When the Mars Observer failed to respond to messages radioed by the ground controllers here on Earth, further efforts to communicate were made-once every 20 minutes. Even though they were met with silence, further attempts were made, less regularly, until the mission was declared a loss on September 27, 1993 and no further attempts to contact were made after that

Propulsion system failure

In 1994, an independent board from the Naval Research Laboratory announced their findings regarding the failure. They suggested that the most probable cause of the communications failure must be a rupture of the fuel pressurisation tank in the propulsion system of the spacecraft

Regardless of what the reason was, an estimated cost of $1 billion, which included the price of the spacecraft along with the costs of space shuttle launching and processing of scientific data was lost. While the science instruments were reflown on two other orbiters, Mars Global Surveyor and 2001 Mars Odyssey, there is no telling if Mars Observer followed the automatic programming to go into Mars orbit flew by the planet, or even if it continues to operate.

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HAVE YOU EVER WONDERED WHAT THE RESTROOM SCENARIO IN SPACE IS LIKE?

On May 5, 1961, barely three weeks after Soviet cosmonaut Yuri Gagarin’s historic orbit of the Earth, NASA astronaut Alan Shepard waited, strapped into the Freedom 7 spacecraft. He would become the first American in space. What NASA officials hadn’t anticipated was that Shepard would have to endure five hours of delay cocooned in his shiny silver spacesuit before his 15-minute orbit.

“Man, I got to pee,” he frantically radioed launch control. Allowing Shepard to urinate in his suit would destroy the medical sensors he was wired with, but eventually launch control had no option but to let him go. Shepard had to suffer the discomfort of a wet suit till the cooling system inside evaporated the liquid.

Early efforts

NASA hadn’t solved the problem entirely even in 1963 when Gordon Cooper blasted off on the last Project Mercury flight. There was a urine collection device inside the suit, but the urine leaked out of the bag and the droplets seeped into the electronics, leading to a systems failure towards the end of the mission.

If wayward pee was a problem, think of what its twin, poop, could do in the cramped quarters of a spacecraft!

The Gemini project was launched to prepare men for the Apollo moon mission. In 1965, Jim Lovell and Frank Borman spent 14 days flying in Gemini 7, the longest manned mission at the time. They had to poop into a cylindrical plastic bag and add a substance to kill the bacteria and odours. Though the pee could be sent out directly into space through a valve-operated hose, the poo bags had to be stored in the craft till they landed.

By the time the Apollo missions came around, the system hadn’t improved much. The Moon men’s toilet ordeal lasted 45 minutes to an hour. They had to undress completely in a corner of the spacecraft and stick a faecal collection bag to their bottom. Low gravity meant that the poop wouldn’t fall down. The astronauts had to manually help it along with a finger cot, a glove-like covering for a single finger. They also had to knead a germicide into it to prevent the growth of gas-forming bacteria that could cause the bags to explode.

Hit and miss

Accidents did happen. Houston once heard the commander of the 1969 Apollo 10 mission Tom Stafford say, “Give me a napkin quick. There’s a turd floating through the air!”

On the first Space Shuttle mission in 1981, astronauts had to unclog smelly blocked toilets. Frozen urine ejected from the Russian Mir space station, damaged the station’s solar panels over time, reducing their effectiveness by around 40%.

Today, on the International Space Station (ISS), each astronaut is given his or her own funnel for peeing. It attaches to a hose. Urine is sent through a filtration system and recycled into drinking water. There is a proper sit down toilet for more serious business. The waste is sucked into a canister, which is stored and later shot back towards Earth along with other trash, where it burns up in the atmosphere.

Did you know?

Astronauts go through ‘positional training’ on Earth to perfect their aim since the toilet on the ISS has a narrow opening. The mock toilet has a camera at the bottom. Astronauts don’t actually go, but watch a video screen in front of them to check that their alignment is spot on. The toilet costs millions of dollars, so missing the target is not an option.

During a spacewalk or an EVA (extravehicular activity), astronauts wear a maximum absorbency garment, which is essentially a large diaper.

NASA’S 2020 Lunar Loo Challenge, which invited designs from the public for compact toilets that would work well in both microgravity and lunar gravity received tremendous response. The Artemis program plans to land a man and the first woman on the Moon by 2024.

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WHERE SHOULD A ROCKET LAUNCHING SITE BE LOCATED?

Many factors are taken into account while choosing a location for a site from where spacecraft are launched. Firstly, the launch site should be at a remote location as far away as possible from populated areas to reduce the chances of human fatalities on the ground in case of a rocket disaster. It is preferable if it is located next to a major water body such as a sea so that parts shed by flying rockets can fall into the open ???an.

The site should be accessible by land, air, and sea to avoid unnecessary transportation costs and delays. Scientists also prefer a site that has pleasant, mild weather conditions.

Launch sites are usually located near the Equator. Earth rotates from west to east. The surface velocity of the rotation is maximum (about 1600 km/hour) at the Equator. A rocket launched in the easterly direction from a site close to the Equator benefits greatly from the natural boost provided by the surface velocity of Earth’s rotation. This cuts down the cost of rockets used to launch satellites that are destined for the geo-stationary orbit, which runs parallel to the Equator. Most launch sites such as the Guiana Space Centre in French Guiana; Cape Canaveral in the U.S.: Sriharikota in Andhra Pradesh; and Thumba in Kerala – are located near the Equator.

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WHO IS BARBARA MORGAN?

On August 8, 2007, space shuttle Endeavour’s STS-118 mission was successfully launched. Among the crew members was Barbara Morgan, the first teacher to travel into space. Barbara Morgan, in full Barbara Radding Morgan, (born Nov. 28, 1951, Fresno, Calif., U.S.), American teacher and astronaut, the first teacher to travel into space. Morgan earned a B.A. in human biology from Stanford University in Palo Alto, Calif., in 1973.

Among the many new things during the COVID-19 pandemic was the school classroom, or the lack of it. During the height of the pandemic in the last two years, students were often seen attending virtual classrooms from homes with the teachers conducting the classes from their houses.

A group of students in the U.S. experienced something similar 15 years ago. Only that their teacher, Barbara Morgan wasn’t teaching virtually from the comfort of her home. Morgan was the first teacher to travel into space and she did do some teaching while in space!

Born in November 1951 in Fresno, California, Morgan obtained a B.A. in human biology from Stanford University in 1973. Having received her teaching credentials by the following year, she began her teaching career in 1974 in Arlee, Montana, teaching remedial reading and maths.

She taught remedial reading, maths, and second grade in McCall, Idaho from 1975-78, before heading to Quito in Ecuador to teach English and science to third graders for a year. Following her return to the U.S., she returned to McCall, Idaho, where she taught second through fourth grades at McCall-Donnelly Elementary School until 1998.

Teacher in Space

Morgan’s tryst with space began in July 1985 when she was selected as the backup candidate for NASA’s Teacher in Space programme. As the backup to American teacher Christa McAuliffe, Morgan spent the time from September 1985 to January 1986 attending various training sessions at NASA’s Johnson Space Center in Houston. After McAuliffe and the rest of the crew died in the 1986 Challenger disaster, Morgan replaced McAuliffe as the Teacher in Space designee and worked with NASA’s education division.

Morgan reported to the Johnson Space Center in August 1998 after being selected by NASA as a mission specialist and NASA’s first educator astronaut. Even though Morgan didn’t participate in the Educator Astronaut Project, the successor to the Teacher in Space programme, NASA gave her the honour of being its first educator astronaut.

Following two years of training and evaluation, Morgan was assigned technical duties. She worked in mission control as a communicator with in-orbit crews and also served with the robotics branch of the astronaut office.

Further delay

Even though she was assigned as a mission specialist to the crew of STS-118 in 2002 and was expected to fly the next year, it was delayed for a number of years following the 2003 Columbia disaster. It was on August 8, 2007 that Morgan finally flew into space on the space shuttle Endeavour on STS-118.

The STS-118 was primarily an assembly-and-repair trip to the International Space Station (ISS). The crew were successfully able to add a truss segment, a new gyroscope, and external spare parts platform to the ISS. Morgan served as loadmaster, shuttle and station robotic arm operator, and also provided support during the spacewalks. All this, in addition to being an educator.

Answers from space

For the first time in human history, school children enjoyed lessons from space, conducted by Morgan. Apart from speaking to the students while in space, she also fielded questions. For one question from a student on how fast a baseball will go in space, she even had another astronaut Clay Anderson throw the ball slowly before floating over to catch it himself. While that opened up the opportunity of playing ball with yourself while in space, she also informed the student that the ball can be thrown fast, but it is avoided in order to not cause any damage to the craft and the equipment on board.

Following the first lessons from space, the Endeavour returned to Earth on August 21 after travelling 5.3 million miles in space. Having carried 5,000 pounds of equipment and supplies to the ISS, it returned with 4,000 pounds worth of scientific materials and used equipment.

As for Morgan, she retired from NASA in 2008 to become the distinguished educator in residence at Boise State University. A post created exclusively for her, it entailed a dual appointment to the colleges of engineering and education. As someone who strongly believes that teachers are learners, she continues to teach and learn, be it from space, or here on Earth.

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WHAT IS THE LUNAR RAINBOW?

A rainbow is a thing of beauty. We know that a rainbow is produced when sunlight is refracted by water droplets in the atmosphere. However, what happens if water droplets reflect and refract moonlight? Simple. We get a moonbow, and no, they aren’t a figment of your imagination.

Moonbows are known as moon rainbow or lunar rainbows. They are much fainter than rainbows because of the lower intensity of moonlight (which is reflected sunlight), and their colours are too faint to be perceived by the human eye. They often appear a ghostly white. However, the colours can be seen through photography. They can be viewed most easily when the Moon is at or nearest to its brightest phase, full-moon. The best time to see moonbows is a couple of hours before sunrise or after sunset. Did you know that they are said to have first been mentioned by Aristotle back in 350BC and that there are certain parts of the world where you are more likely to see them, such as Hawaii?

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WHICH STAR BECAME THE FIRST STAR OTHER THAN OUR SUN TO BE PHOTOGRAPHED?

Vega became the first star other than our sun to be photographed. Visible in the summer sky of the northern hemisphere, Vega is a bright star located about 25 light years from our Earth. On July 16-17, 1850, The days when we could look up to see star-studded skies feel like they are numbered. Especially in cities, as the light pollution makes it impossible for us to enjoy the celestial show. Some stars, however, shine bright enough such that they can be seen even on a moonlit night or from light-polluted cities.

Vega is one such star visible in the summer sky of the northern hemisphere. The brightest star in the constellation Lyra, it is also known as Alpha Lyrae. The fifth-brightest star visible from Earth, it is also among the closest of all bright stars at about 25 light years away.

The Summer Triangle

Along with two other stars – the distant Deneb and the fast-spinning Altair-the blue-white Vega forms an asterism known as the Summer Triangle. These three stars are usually the first to light up the eastern half of the sky after sunset.

Beginning around June and until the end of the year the Summer Triangle pattern can be discerned in the evening every day. Vega, which sinks below the horizon for just seven hours each day, can actually be seen on any day of the year. At mid-northern latitudes on midsummer nights, Vega is usually directly overhead.

The blue-white light of Vega is so bright that it has been observed through the centuries. Be it the Hindus, Chinese, or the Polynesians, the star features prominently in many ancient cultures. Its name, meanwhile, comes from the Arabic word wagi, which means “falling” or “swooping”

First to be photographed

The brightness has meant that Vega has remained relevant in modern times as well, notching up a number of firsts. The first of those firsts came in 1850, when Vega became the first star to be photographed, other than our sun.

On July 16-17, 1850, a 15-inch (38 cm) refractor at the Harvard College Observatory was employed to capture it. Harvard’s first astronomer, William Cranch Bond, had been dabbling with celestial photography at the behest of John Adams Whipple, an American inventor and photographer. Using the daguerreotype process, the duo achieved a 90-second exposure of Vega that yielded the first photograph of a star other than our own. Bond and Whipple, in fact, kept at it and their daguerreotype of the moon the next year created quite a stir at the international exhibition held in London’s Crystal Palace.

Spectrum of a star

A couple of decades later, Vega was again central to another first. Henry Draper, an American doctor and amateur astronomer, was a pioneer in astrophotography. He chose Vega as his subject when he created the first spectrographic image of the star in 1872. Breaking down Vega’s light to reveal the various elements making up the star, Draper had taken the first spectrum of a star other than our sun.

Late in the 1990s, Vega rose to prominence once again after American astronomer Carl Sagan’s novel “Contact” was made into a Hollywood movie. As the movie showed an astronomer discovering a signal appearing to come from Vega while searching for extraterrestrial intelligence, the star captured popular imagination.

Vega’s blue-white light indicates surface temperatures of about 9,400 degree Celsius, much hotter than that of our sun (4,000 degree Celsius). Vega’s diameter is nearly 2.5 times that of the sun, while its mass is also more than twice that of our sun.

Vega is only about 450 million years old, making it a youngster when compared to our sun, which is 4.6 billion years old. Despite Vega being a 10th of the sun’s age, both stars are classified as middle-aged as they are halfway through their respective lives. This means that while our sun will run out of fuel only after another 5 billion years, Vega will burn for only another half-a-billion years.

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MYSTERIES OF THE UFO (UNIDENTIFIED FLYING OBJECTS)

Whether it is the possibility of making contact with alien life, or the mere thrill of the unknown, UFOs have always intrigued us.

It’s a bird. It’s a plane. It’s a UFO! Unidentified Flying Objects or UFOS are exactly the stuff that legends are made of, and have since time immemorial held people in its thrall. From conspiracy theories of their sightings, portrayal in books and movies, their link to alien invasions, and more, have ensured that the topic has remained relevant even with the change of governments and lapse of time.  Naturally, a day dedicated to these mysterious flying saucers was just waiting to happen. Earlier, June 24 was allotted as the day of celebration, for, according to aviator Kenneth Arnold, it was on that day that nine unidentified objects had flown over Washington in the 1990s. However, July 2 was officially allotted as World UFO Day to commemorate the supposed UFO crash incident that occurred in Roswell, New Mexico, in 1947.

The Rosewell Incident It famously refers to the 1947 recovery of balloon debris from a ranch near Corona, New Mexico, by U.S.Army Air Forces officers from the Roswell Army Air Field, and conspiracy theories which emerged decades later, claiming that the debris involved a flying saucer and that the truth had been hushed up by the US government.

Throughout 1947, people across the U.S.. and other countries had been reporting sightings of strange objects in the sky and claiming that. they were alien-piloted spacecrafts In the midst of this the flying saucer furore, in July that year, some unusual material fell on the ground near Roswell. Soon after, an information officer at the Roswell Army Air Field (RAAF) issued an unauthorised press release stating that a flying disk” had been retrieved from a local ranch. The Roswell Daily Record immediately printed the story headlined “RAAF Captures Flying Saucer On Ranch in Roswell Region”

The officer was admonished and the Army duly retracted the statement and said that the crashed object was a conventional weather balloon. While the incident slowly died down, it eventually laid the ground for several hoaxes in the future.

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WHAT IS JAMES WEBB TELESCOPE?

NASA’s James Webb Space Telescope (JWST) is an infrared space observatory that launched on Dec 25, 2021, from ESA’s launch site at Kourou in French Guiana, at 7:20 a.m. EST (1220 GMT; 9:20 a.m. local time in Kourou), aboard an Arianespace Ariane 5 rocket.

NASA released the first scientific images from Webb at a live event on July, 12. Explore the first images in more detail and what it means for JWST science in our recently published article.

The $10 billion James Webb Space Telescope — NASA’s largest and most powerful space science telescope — will probe the cosmos to uncover the history of the universe from the Big Bang to alien planet formation and beyond. It is one of NASA’s Great Observatories, huge space instruments that include the likes of the Hubble Space Telescope to peer deep into the cosmos.

The release of the first full-colour images and spectroscopic data will mark the beginning of the next era in astronomy as Webb will help answer questions about the earliest moments of the universe and allow astronomers to study exoplanets in greater detail than ever before. James Webb was launched in December to succeed the revolutionary – but now ageing-Hubble Space Telescope. The James Webb Space Telescope uses a 19.7-foot-tall primary mirror to collect light. That light is bounced to a smaller secondary mirror, which then redirects it onto the telescope’s instruments, including a camera that records an image.

While Hubble looks mostly in the visual and ultraviolet parts of the electromagnetic spectrum, Webb will look at longer wavelengths in the infrared, to see what the universe looked like around 100 to 250 million years after the Big Bang, when the first stars and galaxies were formed.

Early alignment imagery already demonstrated the unprecedented sharpness of Webb’s infrared view. However, these new images will be the first in full colour and the first to showcase Webb’s full science capabilities.

Credit : Space.com 

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WHO WAS THE FIRST AMERICAN WOMAN TO WALK IN SPACE?

On June 18, 1983, Sally K. Ride was onboard the space shuttle Challenger for the STS-7 mission, thereby becoming the first American woman to go into space. Apart from making two space flights, Ride championed the cause of science education for children.

The first decades of space exploration was largely dominated by two countries the US and the Soviet Union This period is even referred to as the Space Race as the two Cold War adversaries pitted themselves: against each other to achieve superior spaceflight capabilities.

While the two countries were neck and neck in most aspects. the Soviets sent a woman to space much before the US. Even though Valentina Tereshkova became the first woman in space in June 1963, it was another 20 years before Sally Ride became the first American woman in space

Urged to explore

Ride was the older of two daughters born  to Carol Joyce Ride and Dale Ride. Even though her mother was a counsellor and her father a professor of political science. Ride credits them for fostering her interest in science by enabling her to explore from a very young age.

An athletic teenager, Ride loved sports such as tennis, running, volleyball, and softball. In fact, she attended Westlake School for Girls in Los Angeles on a partial tennis scholarship. She even tried her luck in professional tennis, before returning to California to attend Stanford University.

By 1973, Ride not only had a Bachelor of Science degree in Physics, but had also obtained a Bachelor of Arts degree in English. She got her Master of Science degree in 1975 and obtained her Ph.D. in Physics by 1978

Restriction removed

Having restricted astronaut qualification to men for decades,  NASA expanded astronaut selection with the advent of the space shuttle from only pilots to engineers and scientists, opening the doorway for women finally. Having seen an ad in a newspaper inviting women to apply for the astronaut programme Ride decided to give it a shot

Out of more than 8,000 applications, Ride became one of six women who were chosen as an astronaut candidate in January 1978. Spaceflight training began soon after and it included parachute jumping, water survival, weightlessness, radio communications, and navigation, among others. She was also involved in developing the robot arm used to deploy and retrieve satellites.

Ride served as part of the ground-support crew for STS-2 and STS-3 missions in November 1981 and March 1982. In April 1982, NASA announced that Ride would be part of the STS-7 crew, serving as a mission specialist in a five-member crew.

First American woman in space

On June 18, 1983, Ride became the first American woman in space. By the time the STS-7 mission was completed and the space shuttle Challenger returned to Earth on June 24, they had launched communications satellites for Canada and Indonesia. As an expert in the use of the shuttle’s robotic arm, Ride also helped deploy and retrieve a satellite in space using the robot arm.

Ride created history once again when she became the first American woman to travel to space a second time as part of the STS-41G in October 1984. During this nine-day mission, Ride employed the shuttle’s robotic arm to remove ice from the shuttle’s exterior and to also readjust a radar antenna. There could have even been a third, as she was supposed to join STS-61M, but that mission was cancelled following the 1986 Challenger disaster.

Even after her days of space travel were over, Ride was actively involved in influencing the space programme. When accident investigation boards were set up in response to two shuttle tragedies – Challenger in 1986 and Columbia in 2003 Ride was a part of them both.

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WHAT IS JUPITER’S IO MOON?

Io or Jupiter I, is the innermost and third-largest of the four Galilean moons of the planet Jupiter. Slightly larger than Earth’s moon, Io is the fourth-largest moon in the Solar System, has the highest density of any moon, the strongest surface gravity of any moon, and the lowest amount of water (by atomic ratio) of any known astronomical object in the Solar System. It was discovered in 1610 by Galileo Galilei and was named after the mythological character Io, a priestess of Hera who became one of Zeus’s lovers.

With over 400 active volcanoes, Io is the most geologically active object in the Solar System.

This extreme geologic activity is the result of tidal heating from friction generated within Io’s interior as it is pulled between Jupiter and the other Galilean moons—Europa, Ganymede and Callisto. Several volcanoes produce plumes of sulfur and sulfur dioxide that climb as high as 500 km (300 mi) above the surface. Io’s surface is also dotted with more than 100 mountains that have been uplifted by extensive compression at the base of Io’s silicate crust. Some of these peaks are taller than Mount Everest, the highest point on Earth’s surface.  Unlike most moons in the outer Solar System, which are mostly composed of water ice, Io is primarily composed of silicate rock surrounding a molten iron or iron sulfide core. Most of Io’s surface is composed of extensive plains with a frosty coating of sulfur and sulfur dioxide.

Io’s volcanism is responsible for many of its unique features. Its volcanic plumes and lava flows produce large surface changes and paint the surface in various subtle shades of yellow, red, white, black, and green, largely due to allotropes and compounds of sulfur. Numerous extensive lava flows, several more than 500 km (300 mi) in length, also mark the surface. The materials produced by this volcanism make up Io’s thin, patchy atmosphere and Jupiter’s extensive magnetosphere. Io’s volcanic ejecta also produce a large plasma torus around Jupiter.

Io played a significant role in the development of astronomy in the 17th and 18th centuries; discovered in January 1610 by Galileo Galilei, along with the other Galilean satellites, this discovery furthered the adoption of the Copernican model of the Solar System, the development of Kepler’s laws of motion, and the first measurement of the speed of light. Viewed from Earth, Io remained just a point of light until the late 19th and early 20th centuries, when it became possible to resolve its large-scale surface features, such as the dark red polar and bright equatorial regions. In 1979, the two Voyager spacecraft revealed Io to be a geologically active world, with numerous volcanic features, large mountains, and a young surface with no obvious impact craters. The Galileo spacecraft performed several close flybys in the 1990s and early 2000s, obtaining data about Io’s interior structure and surface composition. These spacecraft also revealed the relationship between Io and Jupiter’s magnetosphere and the existence of a belt of high-energy radiation centered on Io’s orbit. Io receives about 3,600 rem (36 Sv) of ionizing radiation per day.

Further observations have been made by Cassini–Huygens in 2000, New Horizons in 2007, and Juno since 2017, as well as from Earth-based telescopes and the Hubble Space Telescope.

Credit : Wikipedia 

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WHICH ASTEROID IS MADE OF METALS?

Nasa has discovered a rare and highly valuable asteroid called ’16 psyche’. It was found by nasa’s hubble space telescope. The asteroid is located in our solar system’s asteroid belt between the planets of mars and jupiter.

According to a study published by the planetary science journal on monday, asteroid ’16 psyche’ is located roughly 370 million kilometres (230 million miles) from the earth and measures 226 kilometres across (140 miles).

The most interesting thing about the asteroid is what it’s made of. Unlike other asteroids made up of either rocks or ice, psyche is made up of metals.

One of the study’s authors tracy becker said that they usually come across meteorites that have metal deposits but since psyche is made up entirely of metals, it is quite unique.

Psyche’s size and presence of metal deposits means that it could be worth $10,000 quadrillion ($10,000,000,000,000,000,000), which is equivalent to ten thousand times the global economy in 2019.

Researchers used the ultraviolet spectrum data collected by the space telescope imaging spectrograph on the hubble telescope during two observations made in 2017.

The data showed them that psyche’s surface could be made of pure iron but they also found that the presence of iron composition as small as 10 percent could dominate ultraviolet reports. Psyche is believed to be the dead core of a planet that might have failed during its formative stages or it could also be the result of many violent space collisions.

Nasa has already targeted the exploration of asteroid psyche with the launch of nasa discovery mission psyche, which is expected to be launched in 2022. The psyche space probe will be sent atop a spacex falcon heavy rocket and will reach the asteroid by 2026, and hopefully uncover its exact metal content and other facets.

Credit :  India times 

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WHY SOMETIMES WE CAN SEE MORE THAN THE CRESCENT MOON?

Although we usually see only the brightly lit part of the moon during its crescent phase, we sometimes see the other part too, though dimly lit.

What’s the reason?

Earth reflects the sun’s light falling on it just like the  moon does. The earth, in fact, is a better reflector than the moon. The oceans which cover three-fourths of the earth’s surface, reflect a lot of solar radiation back into space. So just as we have moonlight here, there is earthlight on the dark side of the moon. It is this earthlight which makes the moon beyond the crescent dimly visible to us.

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HOW DO ASTRONAUTS COMMUNICATE IN SPACE?

Sound can only travel through a solid, liquid or gas and not through vacuum. As there is near complete vacuum in space, sound cannot travel and be heard through the ears like on Earth. Other forms of electromagnetic radiation including radio waves, however, can travel through vacuum. When astronauts are in a space shuttle or a space station, they can speak normally there are enough air particles to vibrate and take the sound to their ear drum. But when they are conducting a spacewalk, they need a special device to communicate with each other The helmets of astronauts are fitted with a device which converts the sound waves generated by their speech into radio waves and transmits them to other astronauts. When the headset of another astronaut receives the radio waves, it translates the signal into the sound form. The same principle is used to send and receive messages from Earth.

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WHAT IS THE SURFACE AROUND A BLACK HOLE THAT REPRESENTS THE DISTNACE OF APPROACH BEYOND WHICH EVEN LIGHT CANNOT ESCAPE?

A black hole is an astronomical object with a gravitational pull so strong that nothing, not even light, can escape it. A black hole’s “surface,” called its event horizon, defines the boundary where the velocity needed to escape exceeds the speed of light, which is the speed limit of the cosmos.

In astrophysics, an event horizon is a boundary beyond which events cannot affect an observer. Wolfgang Rindler coined the term in the 1950s. In 1784, John Michell proposed that gravity can be strong enough in the vicinity of massive compact objects that even light cannot escape. At that time, the Newtonian theory of gravitation and the so-called corpuscular theory of light were dominant. In these theories, if the escape velocity of the gravitational influence of a massive object exceeds the speed of light, then light originating inside or from it can escape temporarily but will return. In 1958, David Finkelstein used general relativity to introduce a stricter definition of a local black hole event horizon as a boundary beyond which events of any kind cannot affect an outside observer, leading to information and firewall paradoxes, encouraging the re-examination of the concept of local event horizons and the notion of black holes. Several theories were subsequently developed, some with and some without event horizons. One of the leading developers of theories to describe black holes, Stephen Hawking, suggested that an apparent horizon should be used instead of an event horizon, saying, “gravitational collapse produces apparent horizons but no event horizons.” He eventually concluded that “the absence of event horizons means that there are no black holes – in the sense of regimes from which light can’t escape to infinity.”

Any object approaching the horizon from the observer’s side appears to slow down, never quite crossing the horizon. Due to gravitational redshift, its image reddens over time as the object moves away from the observer.

Credit : Wikipedia 

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WHAT IS THE DIFFERENCE BETWEEN CONSTELLATIONS AND ASTERISMS?

Constellations are the 88 recognized patterns and groups of stars. These groups and patterns are usually associated with mythology. Today, constellations are not only the groups of stars, but now refers to the entire region of the sky that it takes up.

Asterisms are groups of stars that do not form their own constellations, but instead, are inside of constellations. The Big Dipper is an example of this. The Big Dipper is an asterism inside of the constellation Ursa Major. So I believe that asterisms are smaller than the constellations that they’re in, but not necessarily bigger than all constellations.

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WHAT IS AN ASTERISM?

An asterism is an observed pattern or group of stars in the sky. Asterisms can be any identified pattern or group of stars, and therefore are a more general concept then the formally defined 88 constellations. Constellations are based on asterisms, but unlike asterisms, constellations outline and today completely divide the sky and all its celestial objects into regions around their central asterisms. For example, the asterism known as the Big Dipper comprises the seven brightest stars in the constellation Ursa Major. Another is the asterism of the Southern Cross, within the constellation of Crux.

Asterisms range from simple shapes of just a few stars to more complex collections of many stars covering large portions of the sky. The stars themselves may be bright naked-eye objects or fainter, even telescopic, but they are generally all of a similar brightness to each other. The larger brighter asterisms are useful for people who are familiarizing themselves with the night sky.

The patterns of stars seen in asterisms are not necessarily a product of any physical association between the stars, but are rather the result of the particular perspectives of their observations. For example the Summer Triangle is a purely observational physically unrelated group of stars, but the stars of Orion’s Belt are all members of the Orion OB1 association and five of the seven stars of the Big Dipper are members of the Ursa Major Moving Group. Physical associations, such as the Hyades or Pleiades, can be asterisms in their own right and part of other asterism at the same time.

Credit : Wikipedia 

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WHICH IS THE SMALLEST CONSTELLATION?

The smallest constellation is Crux, the Southern Cross. A small group of four bright stars that forms a Latin cross in the southern sky, Crux is visible from latitudes south of 25 degrees north and completely invisible in latitudes above 35 degrees north (in the United States, roughly north of Texas).

Originally it was part of the constellation Centaur, but became its own constellation during the 16th century when it was used as a valuable navigation tool by explorers. Its area is calculated at about 68 square degrees.

Blue-white ? Crucis (Acrux) is the most southerly member of the constellation and, at magnitude 0.8, the brightest. The three other stars of the cross appear clockwise and in order of lessening magnitude: ? Crucis (Mimosa), ? Crucis (Gacrux), and ? Crucis (Imai). ? Crucis (Ginan) also lies within the cross asterism. Many of these brighter stars are members of the Scorpius–Centaurus association, a large but loose group of hot blue-white stars that appear to share common origins and motion across the southern Milky Way.

Crux contains four Cepheid variables, each visible to the naked eye under optimum conditions. Crux also contains the bright and colourful open cluster known as the Jewel Box (NGC 4755) on its eastern border. Nearby to the southeast is a large dark nebula spanning 7° by 5° known as the Coalsack Nebula, portions of which are mapped in the neighbouring constellations of Centaurus and Musca.

Credit : Wikipedia 

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WHICH IS THE LARGEST CONSTELLATION?

Hydra is the largest of the 88 modern constellations, measuring 1303 square degrees, and also the longest at over 100 degrees. Its southern end borders Libra and Centaurus and its northern end borders Cancer. It was included among the 48 constellations listed by the 2nd century astronomer Ptolemy. Commonly represented as a water snake, it straddles the celestial equator.

Despite its size, Hydra contains only one moderately bright star, Alphard, designated Alpha Hydrae. It is an orange giant of magnitude 2.0, 177 light-years from Earth. Its traditional name means “the solitary one”. Beta Hydrae is a blue-white star of magnitude 4.3, 365 light-years from Earth. Gamma Hydrae is a yellow giant of magnitude 3.0, 132 light-years from Earth.

Hydra has one bright binary star, Epsilon Hydrae, which is difficult to split in amateur telescopes; it has a period of 1000 years and is 135 light-years from Earth. The primary is a yellow star of magnitude 3.4 and the secondary is a blue star of magnitude 6.7. However, there are several dimmer double stars and binary stars in Hydra. 27 Hydrae is a triple star with two components visible in binoculars and three visible in small amateur telescopes. The primary is a white star of magnitude 4.8, 244 light-years from Earth. The secondary, a binary star, appears in binoculars at magnitude 7.0 but is composed of a magnitude 7 and a magnitude 11 star; it is 202 light-years from Earth. 54 Hydrae is a binary star 99 light-years from Earth, easily divisible in small amateur telescopes. The primary is a yellow star of magnitude 5.3 and the secondary is a purple star of magnitude 7.4. N Hydrae (N Hya) is a pair of stars of magnitudes 5.8 and 5.9. Struve 1270 (?1270) consists of a pair of stars, magnitudes 6.4 and 7.4.

The other main named star in Hydra is Sigma Hydrae (? Hydrae), which also has the name of Minchir, from the Arabic for snake’s nose. At magnitude 4.54, it is rather dim. The head of the snake corresponds to the ?shlesh? Nakshatra, the lunar zodiacal constellation in Indian astronomy. The name of Nakshatra (Ashlesha) became the proper name of Epsilon Hydrae since 1 June 2018 by IAU.

Hydra is also home to several variable stars. R Hydrae is a Mira variable star 2000 light-years from Earth; it is one of the brightest Mira variables at its maximum of magnitude 3.5. It has a minimum magnitude of 10 and a period of 390 days. V Hydrae is an unusually vivid red variable star 20,000 light-years from Earth. It varies in magnitude from a minimum of 9.0 to a maximum of 6.6. Along with its notable color, V Hydrae is also home to at least two exoplanets. U Hydrae is a semi-regular variable star with a deep red color, 528 light-years from Earth. It has a minimum magnitude of 6.6 and a maximum magnitude of 4.2; its period is 115 days.

Hydra includes GJ 357, an M-type main sequence star located only 31 light-years from the Solar System. This star has three confirmed exoplanets in its orbit, one of which, GJ 357 d, is considered to be a “Super-Earth” within the circumstellar habitable zone.

Credit : Wikipedia 

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HOW MANY CONSTELLATIONS ARE RECOGNIZED BY INTERNATIONAL ASTRONOMICAL UNION?

There are 88 modern constellations recognized by the International Astronomical Union (IAU). The list of the modern constellations was adopted by the IAU in 1922. The constellation boundaries as we know them today were set in the late 1920s. 36 modern constellations lie principally in the northern celestial hemisphere, while 52 are found in the southern sky.

The list of the modern constellations and the abbreviations used for them were produced by American astronomer Henry Norris Russell and approved by the IAU in May 1922. Russell’s list corresponded to the constellations listed in the Revised Harvard Photometry star catalogue, published by Harvard College Observatory in 1908. The constellation boundaries were drawn by Belgian astronomer Eugène Delporte and officially adopted in 1928.

The 88 modern constellations have different origins. Most of them are roughly based on the 48 ancient constellations catalogued by the Greek astronomer Claudius Ptolemy of Alexandria in his Almagest, an ancient astronomical treatise written in the 2nd century CE. These constellations are mostly associated with figures from Greek mythology. They include Andromeda, Cassiopeia, Perseus, Pegasus, Hercules, Orion, Ursa Major, Ursa Minor, Canis Major, Canis Minor, Eridanus, and the 12 zodiac constellations.

However, Ptolemy did not create these constellations. They were already well-known to observers long before his time. Even though they are called Greek constellations, they were not necessarily created by the Greeks. Depictions of some of the ancient constellations or the asterisms they are known for go back to prehistoric times and their creators are unknown.

Fifty of the modern 88 constellations are based on the Greek ones. Only one of Ptolemy’s constellations – Argo Navis – is no longer in use. Once the largest constellation in the sky, Argo Navis represented the ship of Jason and the Argonauts. It was divided into three smaller constellations – Carina, Puppis and Vela – by the French astronomer Nicolas-Louis de Lacaille in the 18th century. The three smaller constellations remain in use.

Credit : Constellation-guide

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WHO WAS THE FIRST WOMAN IN SPACE?

The first woman to travel in space was Soviet cosmonaut, Valentina Tereshkova. On 16 June 1963, Tereshkova was launched on a solo mission aboard the spacecraft Vostok 6. She spent more than 70 hours orbiting the Earth, two years after Yuri Gagarin’s first human-crewed flight in space.

Tereshkova was born on 6 March 1937 in the village of Bolshoye Maslennikovo in central Russia. Her mother was a textile worker, and her father was a tractor driver who was later recognised as a war hero during World War Two. At the time of his death on the Finnish front, Tereshkova was only two years old.

After leaving school, Tereshkova followed her mother into work at a textile factory. Her first appreciation of flying was going down rather than up when she joined a local skydiving and parachutist club. It was her hobby of jumping out of planes that appealed to the Soviets’ space programme committee. On applying to the cosmonaut corps, Tereshkova was eventually chosen from more than 400 other candidates.

Tereshkova received 18 months of severe training with the Soviet Air Force after her selection. These tests studied her abilities to cope physically under the extremes of gravity, as well as handle challenges such as emergency management and the isolation of being in space alone. At 24 years old, she was honourably inducted into the Soviet Air Force. Tereshkova still holds the title as the youngest woman, and the first civilian to fly in space.

While Tereshkova remains the only woman to have flown solo in space, her mission was a dual flight. Fellow cosmonaut Valeriy Bykovsky launched on Vostok 5 on 14 June 1963. Two days later, Tereshkova launched. The two spacecraft took different flight paths and came within three miles of each other. The cosmonauts exchanged communications while making 48 orbits of Earth, with Tereshkova responding to Bykovsky via her callsign ‘Seagull’. During the flight, the Soviet state television network broadcast a video of Tereshkova inside the capsule, and she spoke with the Russian Premier Nikita Khrushchev over the radio.

In her later life, Tereshkova was decorated with prestigious medals and has held several prominent political positions both for the Russian and global councils. Before the collapse of the Soviet Union, she was an official head of State and was elected a member of the World Peace Council in 1966.

Today, she holds the position of Deputy Chair for the Committee for International Affairs in Russia. She also remains active within the space community and is quoted as suggesting that she would like to fly to Mars – even if it were a one-way trip.

Credit : Royal  museums greenwich

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WHY DOES A SHADOW PASS OVER THE MOON DURING A LUNAR ECLIPSE?

When the Moon passes between Sun and Earth, the lunar shadow is seen as a solar eclipse on Earth. When Earth passes directly between Sun and Moon, its shadow creates a lunar eclipse. Lunar eclipses can happen only when the Moon is opposite the Sun in the sky, a monthly occurrence we know as a full Moon. Lunar eclipses can happen only when the Moon is opposite the Sun in the sky, a monthly occurrence we know as a full Moon. But lunar eclipses do not occur every month because the Moon’s orbit is tilted five degrees from Earth’s orbit around the Sun, so most of the time the Moon passes above or below the shadow. Without the tilt, lunar eclipses would occur every month.

Lunar and solar eclipses occur with about equal frequency. Lunar eclipses are more widely visible because Earth casts a much larger shadow on the Moon during a lunar eclipse than the Moon casts on Earth during a solar eclipse. As a result, you are more likely to see a lunar eclipse than a solar eclipse.

Credit : Stardate 

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WHY DOES A COMET HAVE A TAIL?

A comet has two tails. One is a dust tail pushed by light from the sun. Wired Science blogger Rhett Allain uses physics to explain how light can push on matter.

There are two tails because there are two ways the comet can interact with the sun. Everyone thinks about light coming from the sun. However, there is also the solar wind. The solar wind is really just charged particles (like electrons and protons) that escape from the sun due to their high velocities. These charged particles then interact with the ionized gas produced from the comet.

The other tail is due to an interaction with the dust produced by the comet and the light from the sun. Really, it is this interaction that I want to talk about.

Credit : Wired.com

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WHAT IS THE FROZEN PART OF COMETS IS CALLED ?

The nucleus is the solid core of a comet consisting of frozen molecules including water, carbon monoxide, carbon dioxide, methane and ammonia as well as other inorganic and organic molecules — dust. According to ESA the nucleus of a comet is usually around 10 kilometers across or less.

Comets are separated into three distinct parts called the tail, nucleus and the coma which ensures its workability. Comets work in the sense that they tend to be more explicit when they come closer to the source of illumination, the Sun. The tail of a comet is made up of three other parts, the ion tail, the hydrogen envelope, and the dust tail. All these are also vital for the movement of the comet both to and from the sun as indicated below.

The nucleus of a comet is made up of ice, gas, dust, and rocks. It is found right at the center of the head of a comet. The nucleus of a comet is often frozen. The part which is occupied by the gas in the comet’s nucleus is made up of carbon dioxide, the carbon monoxide, ammonia, and methane.

The comet’s area which is made up of the nucleus encompasses between 0.6 to around 6 miles. At times, it is even more than this distance. The nucleus, following this combination of materials, carries the most mass of the comet. The nucleus of a comet is also regarded as one of the darkest objects ever witnessed in the space.

Credit : Earth eclipse

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WHAT IS IT CALLED WHEN A COMET IS CLOSEST TO THE SUN?

Coma. As a comet gets closer to the sun, the ice on the surface of the nucleus begins turning into gas, forming a cloud around the comet known as the coma. According to science website howstuffworks.com the coma is often 1,000 times larger than the nucleus. Outside the coma is a layer of hydrogen gas called a hydrogen halo which extends up to 1010 meters in diameter. The solar wind then blows these gases and dust particles away from the direction of the Sun causing two tails to form. These tails always point away from the Sun as the comet travels around it. One tail is called the ion tail and is made up of gases which have been broken apart into charged molecules and ions by the radiation from the Sun. Since the most common ion, CO+ scatters the blue light better than red light, to observers, this ion tail often appears blue.

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HOW MANY COMETS HAVE BEEN IDENTIFIED SO FAR?

The current number of known comets is: 3,743. Comets are frozen leftovers from the formation of the solar system composed of dust, rock, and ices. They range from a few miles to tens of miles wide, but as they orbit closer to the Sun, they heat up and spew gases and dust into a glowing head that can be larger than a planet. This material forms a tail that stretches millions of miles.

Comets are cosmic snowballs of frozen gases, rock, and dust that orbit the Sun. When frozen, they are the size of a small town. When a comet’s orbit brings it close to the Sun, it heats up and spews dust and gases into a giant glowing head larger than most planets. The dust and gases form a tail that stretches away from the Sun for millions of miles. There are likely billions of comets orbiting our Sun in the Kuiper Belt and even more distant Oort Cloud.

Credit : NASA science 

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HAS ANYONE EVER PLAYED GOLF ON THE MOON?

Yes, that credit goes to American astronaut Alan Shepard. He was the first to play golf on the lunar surface. He achieved the feat when he was part of the Apollo 14 mission in 1971. He is said to have hit two golf balls across the surface of the moon with a makeshift club.

Shepard took a few moments during the Apollo 14 landing to show off his hobby during a live broadcast from the lunar surface on Feb. 6, 1971. He took two shots, with the second ball going “miles and mile,” he said on-camera. He was exaggerating, according to new analysis from the United States Golf Association (USGA). Based on data from the crew and a modern-day moon mission, the group found that the first ball traveled 24 yards (22 meters) and the second about 40 yards (37 m). By comparison, a 2019 report using golf tournaments’ gender categories shows that an average amateur male golfer on Earth can drive the ball 216 yards (198 m), and an average female golfer 148 yards (135 m), although those distances have increased significantly since Shepard’s flight. To be fair to Shepard, however, he had more obstacles to contend with than your typical Sunday hobbyist. His golf “club” was actually a modified sample collection device with the head attached to the end. He was also wearing a notoriously stiff spacesuit that forced him to swing with a single arm.

USGA found the lunar golf balls in high-resolution, enhanced scans of the original flight footage of the Apollo 14 mission. The association measured the point between divot and locations where the balls ended up using high-resolution images from orbit taken by NASA’s Lunar Reconnaissance Orbiter, which launched in 2009.

The association used a second technique to confirm the measurements. Some of the images used were photo sequences taken from the lunar module, the astronauts’ landing craft, taken to show the entire landing site to geologists on Earth. USGA stitched the photographs into a panorama to demonstrate the location of the divot and the two balls, which (after taking the new photo enhancements into account) were well within view of the landed spacecraft.

The two balls are also visible in Apollo 14 takeoff footage, but only after applying “a complex stacking technique on multiple separate frames,” according to a USGA Golf Journal story. This means NASA astronauts Shepard and Ed Mitchell likely couldn’t have seen the balls themselves from the spacecraft, either during their time on the ground or when flying away from the moon.

Credit : Space.com

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What is a Sungrazing Comet?

Sungrazing comets are a special class of comets that come very close to the sun at their nearest approach, a point called perihelion. To be considered a sungrazer, a comet needs to get within about 850,000 miles from the sun at perihelion. Many come even closer, even to within a few thousand miles.

Being so close to the sun is very hard on comets for many reasons. They are subjected to a lot of solar radiation which boils off their water or other volatiles. The physical push of the radiation and the solar wind also helps form the tails. And as they get closer to the sun, the comets experience extremely strong tidal forces, or gravitational stress. In this hostile environment, many sungrazers do not survive their trip around the sun. Although they don’t actually crash into the solar surface, the sun is able to destroy them anyway.

Many sungrazing comets follow a similar orbit, called the Kreutz Path, and collectively belong to a population called the Kreutz Group. In fact, close to 85% of the sungrazers seen by the SOHO satellite are on this orbital highway. Scientists think one extremely large sungrazing comet broke up hundreds, or even thousands, of years ago, and the current comets on the Kreutz Path are the leftover fragments of it. As clumps of remnants make their way back around the sun, we experience a sharp increase in sungrazing comets, which appears to be going on now. Comet Lovejoy, which reached perihelion on December 15, 2011 is the best known recent Kreutz-group sungrazer. And so far, it is the only one that NASA’s solar-observing fleet has seen survive its trip around the sun.

Comet ISON, an upcoming sungrazer with a perihelion of 730,000 miles on November 28, 2013, is not on the Kreutz Path. In fact, ISON’s orbit suggests that it may gain enough momentum to escape the solar system entirely, and never return. Before it does so, it will pass within about 40 million miles from Earth on December 26th. Assuming it survives its trip around the sun.

Credit : Goddard Media Studios 

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DOES THE TEMPERATURE OF NEPTUNE CHANGE?

Neptune, the farthest planet in the solar system, takes more than 165 years to complete an orbit around the sun. As Neptune has an axial tilt, it experiences seasons, just like our Earth.

Sensing emitted heat : Neptune’s great distance from the sun and the longer period of revolution, however, implies that its seasons change slowly, lasting over 40 Earth years each. A new research published in April in Planetary Science Journal revealed that the temperatures in Neptune’s atmosphere have fluctuated unexpectedly over the last two decades, even though this period only represents half of a Neptune season.

An international team of researchers that included scientists from Leicester and NASA’s Jet Propulsion Laboratory used observations that effectively sensed heat emitted from Neptune’s atmosphere. They combined two decades worth of thermal infrared images of Neptune from the European Southern Observatory’s Very Large Telescope; Gemini South telescope in Chile; Subaru Telescope, Keck Telescope, and the Gemini North Telescope in Hawaii; and spectra from NASA’s Spitzer Space Telescope.

Cooler than we thought :  Analysing this data allowed the researchers to reveal a complete picture of trends in Neptune’s temperatures like never before, and some of these revelations were unexpected, to say the least. Since the beginning of reliable thermal  imaging of Neptune in 2003, the datasets indicate a decline in Neptune’s thermal brightness, which came as a surprise to the researchers. This means that the globally averaged temperature in Neptune’s atmosphere has come down by almost 8 degrees Celsius from 2003 to 2018, making the planet cooler than what we thought  before.

The data from Neptune’s south pole, however, reveals a different dramatic change. Observations of this region show that Neptune’s polar stratosphere has warmed up by nearly 11 degrees Celsius from 2018 to 2020, reversing the previous cooling trend.

As of now, the causes for these stratospheric temperature changes are unknown and follow-up observations of the temperature will be needed to further assess these findings. Some of those causes might be revealed by the James Webb Space Telescope that is set to observe both Uranus and Neptune later this year.

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What is the longest drive record Perseverance Mas rover has set?

NASA’s Perseverance Mars rover set a new record for the longest drive in a single Martian day, travelling 245.76 metres (806 feet) on the surface of Mars on February 4. The previous record was held by NASA’s Opportunity rover in 2005 (214 metres/702 feet). Perseverance broke a second record, surpassing its own longest AutoNav drive. NASA integrated this function into a rover for the first time. When in AutoNav, the rover drives autonomously by navigating through 3D maps and software that help it avoid obstacles. This feature makes Perseverance faster as compared to when it’s being remotely controlled by NASA personnel; it would only traverse about 200 metres a day which would lengthen the timeline of exploration. Perseverance landed on the red planet a year ago and is on a mission to seek out signs of ancient microbial life. It has collected six samples of Martian rock and atmosphere, over 50GB of science data and has sent back over 100,000 images. It has also snapped two selfies on the Martian surface!

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Where are most meteorites found?

Researchers from Delft University of Technology in The Netherlands have used artificial intelligence to create a treasure map of zones in which to find meteorites hidden in Antarctic ice.

Sixty-two per cent of all meteorites recovered on Earth were found in Antarctica, making this cold continent a hotbed for space research. These meteorites provide a unique view into the origin and evolution of the solar system.

Meteorites have been accumulating in Antarctica for millennia, falling from space and becoming embedded in ice sheets within the continent’s interior. As the glaciers slowly flow, the meteorites are carried with them. If a glacier comes up against a large obstacle, in areas like the Transantarctic Mountains, the ice rises and meteorites are brought to the surface. Dry Antarctic winds gradually erode the ice, exposing the meteorites. As more ice rises to the surface, the process repeats. Given enough time, a significant accumulation of meteorites builds up.

Researchers say that satellite observations of temperature, ice flow rate, surface cover and geometry are good predictors of the location of meteorite rich areas, and expect the “treasure map’ to be 80 per cent accurate. Based on the study, scientists calculate that as many as 300,000 meteorites are out there on the Antarctic landscape.

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Why do the footprints of astronauts remain unchanged on the surface of the moon?

We are pretty proud of the human flight to the Moon and our footprints on the lunar surface. But did you know these footprints can last a million years on the surface of the Moon? It has been decades since humans last set foot on the Moon, but its surface is still marked with the historic footprints of the 12 astronauts who walked across it Unlike on Earth, there is no erosion by wind or water on the Moon because it has no atmosphere. The Moon is geologically inactive there are no earthquakes or volcanoes. So, nothing gets washed away and nothing gets eroded.

However, the Moon is exposed to bombardment by meteorites, which change the surface. One little spacerock could easily wipe out a footprint on the moon. And since the Moon has no atmosphere, it is exposed to the solar wind, a stream of charged particles coming from the sun, and over time this acts almost like weather on Earth to scour surfaces on the moon, but the process is very, very slow.

On July 20, 1969, Neil Armstrong put his left foot on the rocky Moon. It was the first human footprint on the Moon. They had taken TV cameras with them. The two astronauts walked on the Moon. They picked up rocks and dirt to bring back to Earth. The astronauts had much work to do. Then, the Eagle went back to meet astronaut Collins. He was in the Command Module working.

When Neil Armstrong and Buzz Aldrin visited the moon 50 years ago, they left roughly 100 objects behind, including a portion of their lunar lander, the American flag and, yes, various kinds of trash. Those objects are still there, surrounded by rugged bootprints marking humanity’s first steps on another world. But that site, called Tranquillity Base, may not be as enduring as the legacy those prints represent.

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What is future of the sun?

Nothing in the Universe is permanent. One of the most profound rules in all the Universe is that nothing lasts forever. With gravitational, electromagnetic and nuclear forces all acting on matter, practically everything we observe to exist today will face changes in the future. Even the stars, the most enormous collections that transform nuclear fuel in the cosmos, will someday all burn out, including our Sun. In about five billion years, the Sun will exhaust the hydrogen fuel in its core and start burning helium, forcing its transition into a red giant star. A red giant is a dying star in the final stages of stellar evolution. When the Sun turns into a red giant, it will expand and engulf the inner planets- possibly even Earth. After spending about one billion years as a red giant, the star will become a white dwarf, packing most of its initial mass into a sphere roughly the size of Earth. It will eventually become a black dwarf.

In about 5 billion years time the Sun will have exhausted all the hydrogen at its core. The core, which by then will consist of helium nuclei, will then shrink and nuclear reactions will take place in a large shell outside the core, rather than the core itself. The outer regions of the Sun will greatly expand and it will become a red giant.

It is unclear exactly how large the Sun will get when it becomes a red giant. Current estimates are that it will expand to 100-250 times its current diameter (ref 2). If we take the lower value, the innermost planet Mercury (but not Venus and the Earth) will be swallowed up by the Sun.  At the higher value, the Earth would also be inside the Sun.

When all of the helium in the core has been converted into carbon, nuclear reactions in the core will once again stop. The Sun will start to convert helium into carbon in a shell outside its core but will become more and more unstable. It will vary widely in brightness as it flares up and ejects some of its outer layers into space and then contracts again. Eventually the whole of the outer regions of the Sun will be blown away forming a glowing shell of plasma called a planetary nebula.

With the lower value, where the Sun expands to 100 times its current radius  value, on Earth the Sun would appear 10,000 times larger than it is today. The surface temperature of the Earth would be around 1500 degrees Celsius, hot enough for it glow a dull red colour. The Earth would have lost its atmosphere long before this and will be a bone dry scorched airless desert on which it will be impossible for life to exist.

Credit : Explaining Science

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Did the fruit flies survive in space?

Fruit flies were the first organisms sent to space. For many years before sending mammals into space, such as dogs or humans, scientists studied Drosophila melanogaster (the common fruit fly) and its reactions to both radiation and space flight to understand the possible effects of space and a zero-gravity environment on humans. Starting in the 1910s, researchers conducted experiments on fruit flies because humans and fruit flies share many genes. On February 20, 1947, fruit flies became the first living and sentient organisms to go to space and return, which paved the way for human exploration. At the height of the Cold War and the Space Race, flies were sent on missions to space with great frequency, allowing scientists to study the nature of living and breeding in space. Scientists and researchers from the Soviet Union and the United States both used fruit flies for their research and missions.

Fruit flies have been used in recent years as the reality of Mars and Moon colonization becomes clearer. These flies further the understanding of the effects of weightlessness on the cardiovascular system, the immune system, and the genes of astronauts. Fruit flies have been invaluable assets to scientific discoveries that humankind have made, especially discoveries about space travel.

Mankind has long admired the heavens and wondered about space. Even after the Space Race was completed, advancements in space travel continued. Researchers continue to study the ability of life to survive in the harsh atmosphere of space, promote commercial development, expand and advance knowledge, and prepare future generations for exploration. Throughout time, Animals in space have ensured suitable conditions for human exploration. Larger animals including dogs, monkeys, cats, mice, and others, have been vital to many excursions, as have insects.

The fruit fly has frequently been utilized for space travel, due to its comparable genetics to that of humans. The short gestation period and quick maturing process allows their continued use. Additionally, a female fruit fly can lay one hundred eggs daily, and each egg requires less than ten days to fully mature. Since three-quarters of its genome compares to other organisms, fruit flies frequently proceed humans in space travel because their entire genetic makeup, including the sex chromosomes, have been sequenced by scientists.

Credit : Wikipedia 

Picture Credit : Google

Freakish wonders of the universe

The universe is full of deep mysteries and even the fraction of what we know is too fascinating for words. This month let’s take a look at some of the amazing yet scary inhabitants out there.

I’m coming to visit you

Black holes form when huge stars collapse and grow, taking up other objects around them. Think of them as giant invisible blenders that can tear apart planets even thousands of miles away. There aren’t black holes anywhere close to our solar system, but did you know that they can actually travel through space? And scarier still, rapidly-moving black holes cannot be detected! Scientists have assured us that space is a big place and black holes are quite rare – so sit back and relax!

A big show off!

Ever heard of gamma ray bursts? Well, they are considered as the brightest electromagnetic events to occur in the universe, so much so, that they can be seen billions of miles away! Are you also wondering how powerful they are? Apparently they emit as much energy in a few seconds that our sun can in 10 billion years! We’re glad that, like black holes, they are rare and far, far away from us.

Lone travellers

We imagine planets going around a star, endlessly orbiting it as long as they live. It turns out that not all planets exist this way. Astronomers have discovered a few Jupiter-sized planets drifting alone, without a place to call home or a star as a boss. They are thought to have been ejected out of their star system due to some massive explosion event. As long as they are not on a trajectory towards Earth, it’s dreamy fun to think about these lonely nomadic travellers.

What a blast!

Earth is like a magnet but its magnetic field is quite weak; an MRI machine can produce a magnetic field thousand times stronger. Since we can put our head in through the MRI machine, we can obviously put up with that magnetic field. But imagine a magnetic field that is a trillion times stronger than that of Earth. That’s the kind of power that a magnetar possesses! Come within 1000 kilometres of a magnetar and the very molecules that make you up can dissolve! Here’s a fun fact to freak you out in 2004, a magnetar located halfway across the Milky Way (500 quadrillion kilometres away) quaked and its effect was felt on the Earth’s upper atmosphere!

Mission Impossible

What if you stepped too close to a black hole but not quite? That’s exactly what hypervelocity stars did! They bolted away from the black hole at superfast speed. Hypervelocity stars were originally binary stars, of which one was captured and gobbled up by the black hole at the centre of our galaxy while the other lucky star was sent rocketing off at a very high speed, obviously very, very glad to escape.

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WHY DOES THE SUN RISE IN THE EAST?

Because Earth is spinning eastwards, the Sun comes up from the ground in the east, and sinks in the west.

Most people know that the Sun “rises in the east and sets in the west”. However, most people don’t realize that is a generalization. Actually, the Sun only rises due east and sets due west on 2 days of the year — the spring and fall equinoxes! On other days, the Sun rises either north or south of “due east” and sets north or south of “due west.”

Each day the rising and setting points change slightly. At the summer solstice, the Sun rises as far to the northeast as it ever does, and sets as far to the northwest. Every day after that, the Sun rises a tiny bit further south.

At the fall equinox, the Sun rises due east and sets due west. It continues on it’s journey southward until, at the winter solstice, the Sun rises are far to the south as it ever does, and sets as far to the southwest.

Many, if not most, prehistoric cultures tracked these rising and settings points with great detail. If they had jagged mountains along the horizon, the exact points could be readily remembered. Without a suitably interesting horizon, standing stones could be arranged to line up with the various rising and setting points. Or, tree poles could replace the standing stones. Or, rock cairns could be used.

Credit: Stanford Solar Centre

Picture credit: Google

What is nebula?

A nebula is a formation in space which is constituted mostly of helium, dust, and other gases in various concentrations. The shape and size of a nebula varies, and as such there can be various types of formations having different sizes. Very often, they are huge in size, and their diameters can be a number of light years across. It is derived from Latin, and as such means a cloud. Nebulae exist in the space between the stars—also known as interstellar space. The closest known nebula to Earth is called the Helix Nebula. It is the remnant of a dying star—possibly one like the Sun. It is approximately 700 light-years away from Earth.

It is not clear how exactly a nebula is formed, but it is believed that they are formed by the collapsing of interstellar medium, which then come together because of the gravitational pull of the particles. Nebula is an important object for observation by researchers, who derive significant information about the formation process of stars and planets. A nebula is capable of exerting a gravitational pull, and the force is derived from the particles which come together to form the nebula. With more particles coming together, not only does the nebula increase in proportion, but its gravitational pull also gathers more power and intensity. A nebula is also believed to be one of the primary stages in the formation of stars. Scientists are of the opinion that a nebula can be used to create a trajectory of stellar evolution. There are various nebulae that are in existence at present, though numerous others may exist in the far-flung corners of space that remain to be observed. Some of the most popular ones are Pelican, Crab, Eagle, and Ring Nebula, with Ring being among the most observed ones on the planet.

Credit : Economic Times

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WHAT MAKES THE SEASONS?

Earth is always tilted the same direction as it orbits the Sun. So when Earth is on one side of the Sun, the northern hemisphere is tilted closer towards the Sun, making it warmer. At the same time, the southern hemisphere is tilted away from the Sun, and is, therefore, colder. When Earth reaches the other side of the Sun, it is the opposite, so it’s winter in the northern hemisphere and summer in the southern.

Seasons happen at different times in different parts of the world. The tilt of the Earth doesn’t change as it rotates around the Sun. But the part of the planet that gets the most direct sunlight does change.

The Northern Hemisphere is tilted away from the Sun from September to March. That means the northern half of the planet doesn’t get as much light and heat from the Sun. This causes autumn and winter. During the same months, the Southern Hemisphere is tilted towards the Sun. That means the southern half of the planet gets spring and summer.

From March to September, the Northern Hemisphere is tilted towards the Sun. So that’s when the northern half of the Earth experiences spring and summer. During the same months, the Southern Hemisphere experiences autumn and winter.
Other planets also have seasons. But the length and intensity of each season varies from planet to planet.

  • On Earth, seasons last between 90 and 93 days.
  • On Venus, seasons last between 55 and 58 days.
  • On Mars, seasons change about once every six months. Summer lasts 199 days and winter lasts 146 days.
  • On Saturn, seasons last about seven years.
  • And if you lived on Neptune, you would have to wait more than 40 years for the seasons to change!

Credit: Let’s talk Science

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WHAT IS THE PRIME MERIDIAN?

This is an imaginary line of 0° longitude that is perpendicular to the equator, and parallel to the axis. It passes through Greenwich in the UK, and divides Earth into eastern and western hemispheres. As it crosses the poles to the opposite side of the globe, the line becomes 180° longitude and is also known as the International Date Line.

The prime meridian is arbitrary, meaning it could be chosen to be anywhere. Any line of longitude (a meridian) can serve as the 0 longitude line. However, there is an international agreement that the meridian that runs through Greenwich, England, is considered the official prime meridian.

Governments did not always agree that the Greenwich meridian was the prime meridian, making navigation over long distances very difficult. Different countries published maps and charts with longitude based on the meridian passing through their capital city. France would publish maps with 0 longitude running through Paris. Cartographers in China would publish maps with 0 longitude running through Beijing. Even different parts of the same country published materials based on local meridians.

Finally, at an international convention called by U.S. President Chester Arthur in 1884, representatives from 25 countries agreed to pick a single, standard meridian. They chose the meridian passing through the Royal Observatory in Greenwich, England. The Greenwich Meridian became the international standard for the prime meridian.

Credit: National geographic

Picture credit: Google

WHAT ARE TIME ZONES?

As Earth spins, different parts of its surface turn towards the Sun at different times – the Sun is always rising in one place and setting in another. So, the time of day varies around the world. When it’s dawn where you live, it’s sunset on the other side of the world. To make it easier to set clocks, the world is split into 24 time zones, one for each hour of the day. As you go east around the world, you put clocks forward by one hour for each zone – until you reach an imaginary line called the International Date Line. If you go further on across the Date Line, you carry on adding hours, but put the calendar back by a day.

A time zone is a region on Earth that uses a uniform time. They are often based on the boundaries of countries or lines of longitude. Greenwich Mean Time (GMT) is the mean solar time at the Royal Observatory located in Greenwich, London, considered to be located at a longitude of zero degrees. Although GMT and Coordinated Universal Time (UTC) essentially reflect the same time, GMT is a time zone, while UTC is a time standard that is used as a basis for civil time and time zones worldwide. Although GMT used to be a time standard, it is now mainly used as the time zone for certain countries in Africa and Western Europe. UTC, which is based on highly precise atomic clocks and the Earth’s rotation, is the new standard of today.

UTC is not dependent on daylight saving time (DST), though some countries switch between time zones during their DST period, such as the United Kingdom using British Summer Time in the summer months.

Most time zones that are on land are offset from UTC. UTC breaks time into days, hours, minutes, and seconds, where days are usually defined in terms of the Gregorian calendar. Generally, time zones are defined as + or – an integer number of hours in relation to UTC; for example, UTC-05:00, UTC+08:00, and so on. UTC offset can range from UTC-12:00 to UTC+14:00. Most commonly, UTC is offset by an hour, but in some cases, the offset can be a half-hour or quarter-hour, such as in the case of UTC+06:30 and UTC+12:45

Credit: calculator.net

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What is doomsday fiction?

Imagine a world wrecked by a natural disaster, devastated by nuclear war, or destroyed by a pandemic. While this may sound all too familiar because of the prevailing COVID-19 pandemic, apocalypse fiction is a literary genre that has existed for many years. A subset of science fiction, apocalyptic and post-apocalyptic fiction, also known as doomsday fiction, imagines what life will be like at the end of the world.

How it began

An apocalypse is an event that results in mass destruction and change. Although apocalyptic themes exist in many religious texts, the 20th and 21st centuries have given rise to this genre. The aftermath of World War I, World War II, and the nuclear arms race proved to be fertile ground for writers and filmmakers to conjure up a world plagued by zombies, murderous robots, climate change and even a nuclear holocaust

Apocalyptic vs Post- Apocalyptic

Apocalyptic and post apocalyptic literature is set in a time period where the earth as we know it is coming to an end. An apocalyptic novel or film tells the story of the end of the world, unfolding during the timeline of the story. For example, the 2004 film, “The Day After Tomorrow shows what happens when a sudden worldwide storm plunges the entire planet into a new ice age. On the other hand, post-apocalyptic works portray life in the wake of a cataclysmic event. They focus on how the characters deal with the consequences of a disaster. A 2007 film “1 am Legend” starring Will Smith, is a good example. It follows Robert Neville, a scientist who is the last human survivor of a plague in the whole of New York, as he attempts to find a way to reverse the effects of the human-made virus.

Popular examples

Books written under this genre can be broadly classified (based on their themes) into post-disaster wastelands zombie apocalypse, nature gone wrong, machines taking over the world, and dystopian worlds. Here are a few examples.

Post-disaster wastelands

  • “The Stand” by Stephen King
  • “The Mad Max” film series by James McCausland and George Miller

Zombie Apocalypse

  • World War Z by Max Brooks
  • “The Walking Dead”, a graphic novel series by Robert Kirkman, Tony Moore, and Charlie Adlard

Dystopian worlds

  • “The Hunger Games” by Suzanne Collins
  • “Divergent” by Veronica Roth

Machines taking over

  • “The Maze Runner by James Dashner
  • The Big Melt” by Ned Tillman

 

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