Category Physics

U.K. LAUNCHES NEW COURSE TO TEACH STUDENTS HOW TO SAVE THE PLANET.

The U.K. will offer a new GCSE (General Certificate for Secondary Education) from September 2025 that will “offer young people a chance to develop a deeper knowledge and understanding of this amazing planet, its environment and how to conserve it,” said education secretary Nadhim Zahawi.

The qualification will allow students to learn about organisms and their environments, as well as environmental and sustainability issues. Students will also develop skills for future careers in conservation, “from understanding how to conserve local wildlife to conducting the fieldwork needed to identify species”

Students learn about environmental issues already; this course will teach them about the history and evolution of species and the impact of life on natural environments.

Teen conservationist and wildlife writer Kabir Kaul, 15, said the course “will give my generation the knowledge and practical skills they need to value and protect the environment around them”.

Picture Credit : Google 

WHICH IS THE FIRST CARBON NEUTRAL VILLAGE IN INDIA?

Palli, a village in Jammu and Kashmir’s border district of Samba, became India’s first “carbon-neutral panchayat on April 24, 2022, with Prime Minister Narendra Modi dedicating to the nation a 500-kilowatt solar plant. Palli, according to the Prime Minister, has shown the way to the country by becoming carbon neutral. But what is carbon neutrality and how can it be achieved? Let’s find out.

What is carbon neutrality?

We all know that carbon dioxide emissions are one of the primary causes of climate change and an increasingly warming planet. Carbon-neutrality is the state of achieving a balance between the greenhouse gases put out into the atmosphere and those removed. The term ‘Net-zero’ is sometimes used instead of carbon neutrality and they broadly mean the same. Increasingly, countries, companies, and organisations have been committing to achieve carbon-neutrality or net-zero carbon emission through measures such as reforestation and artificial carbon sequestering. But some environmental activists have criticised such offsetting measures as an excuse to continue polluting. If you’ve been wondering about the benefits of achieving carbon neutrality, there are many such as less pollution, improved air quality, better health and environment, green jobs, reducing the impact of climate change, and a greener planet.

How can it be achieved?

Carbon neutrality can be achieved by reducing the use of fossil fuels and by adopting renewable energy sources, by developing energy-efficient technologies, by adopting massive reforestation or tree-planting measures and by investing in technologies such as carbon sequestration that can remove carbon from the atmosphere. By the way, carbon sequestration is the process of capturing and storing atmospheric carbon dioxide underground permanently and safely. However, no technology or quantity of trees planted could offset the emissions currently generated globally, unless every country and every household is part of this solution.

Palli’s feat

The unassuming village of Palli has made history by becoming India’s first carbon-neutral solar village. It has achieved this feat with the installation of a 500-kilowatt solar plant. According to reports, the project was finished in record time (of nearly three weeks) at a cost of Rs. 2.75 crore. Under the central government’s ‘Gram Urja Swaraj’ programme, as many as 1,500 solar panels put up on an area of 6,408 square metres will provide clean electricity to 340 homes in the model panchayat.

The green energy generated will be distributed to the village through the local power grid station, which has a daily requirement of 2,000 units.

Picture Credit : Google 

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 

Picture Credit : Google 

WHAT WAS THE MERCURY SEVEN MISSION?

On May 15, 1963, the last mission of Project Mercury got under way. Astronaut Gordon Cooper closed out things in style as his flight stretched the capabilities of the Mercury spacecraft to its limits.

The Mercury Seven, also referred to as the Original Seven, were a group of seven astronauts selected to fly spacecraft for Project Mercury – the first human space flight program by the U.S. Even though there were some hiccups, the project, initiated in 1958, was largely successful in its three goals of operating a human spacecraft. investigating an astronaut’s ability to work in space, and recovering spacecraft and crew safely.

Youngest of the Mercury Seven

The final flight of Project Mercury took place in May 1963. The youngest of the Original Seven, astronaut Gordon Cooper, went on to become the first American to fly in space for more than a day during this mission.

Leroy Gordon Cooper Jr. was born in 1927 and served in the Marine Corps in 1945 and 1946. He was commissioned in the U.S. Army after attending the University of Hawaii.

He was called to active duty in 1949 and completed pilot training in the U.S. Air Force. He was a fighter pilot in Germany from 1950 to 1954 and earned a bachelor’s degree at the Air Force Institute of Technology in 1956. He served as a test pilot at Edwards Air Force Base in California until he was selected as an astronaut for Project Mercury. Cooper flew Mercury-Atlas 9, the last Mercury mission, which was launched on May 15, 1963. He called his capsule Faith 7, the number indicating his status as one of the Original Seven astronauts.

Conducts 11 experiments

Longer than all of the previous Mercury missions combined. Cooper had enough time in his hands to conduct 11 experiments. These included monitoring radiation levels, tracking a strobe beacon that flashed intermittently, and taking photographs of the Earth.

When Cooper sent back black-and-white television images back to the control centre during his 17th orbit, it was the first TV transmission from an American crewed spacecraft. And even though there were plans for Cooper to sleep as much as eight hours, he only managed to sleep sporadically during portions of the flight. After 19 orbits without a hitch, a faulty sensor wrongly indicated that the spacecraft was beginning re-entry. A short circuit then damaged the automatic stabilisation and control system two orbits later. Despite these malfunctions and the rising carbon dioxide levels in his cabin and spacesuit. Cooper executed a perfect manual re-entry.

Lands without incident Cooper had clocked 34 hours and 20 minutes in space, orbiting the Earth 22 times and covering most of the globe in the process. This meant that he could practically land anywhere in the globe, a potential pain point that the U.S. State

Department was nervous about. In fact, on May 1, 1963, the country’s Deputy Under Secretary fuel, venting gas that made the spacecraft roll, and more in what felt like a never-ending series during their eight-day mission. They, however, completed 122 orbits, travelling over 5.3 million km in 190 hours and 56 minutes, before safely making their way back to Earth.

After accumulating more than 225 hours in space, Cooper served as the backup command pilot of Gemini 12, which was launched in November 1966, and the backup command pilot for Apollo 10 in May 1969. By the time Cooper left NASA and retired from the Air Force in July 1970, human beings had set foot on the moon, further vindicating the Mercury and Gemini projects that Cooper had been involved with.

Picture Credit : Google 

DO BACTERIA AND FUNGI SPEED UP WEATHERING?

When water collects in the cracks of a rock, it can freeze when temperatures drop. The ice expands and the pressure can split the rock. In cold, mountain regions, one can even hear gunshot-like cracks as rocks are split apart by frost.

A mechanical process, freeze-thaw weathering causes the ?joints?(cracks) in rocks to expand, which wedges parts of rocks apart. Because water expands by about 10% when it freezes, this creates outward pressure in rock joints, making the cracks larger.

Joints occur naturally in rocks as a result of their formation. Fractures that are not offset, joints do allow for the entry of water into rocks.

In climates where temperatures dip below freezing in the winter, moisture in the joints of rocks solidifies as ice. Over time, after several cycles of freezing and thawing, joints get large enough that bit of rock start to fall off in smaller pieces. This breakdown of rock happens faster at higher altitudes, where many freeze-thaw cycles can occur during the year.

Credit: Sciencing

Picture Credit : Google 

HOW DOES FROST BREAK UP ROCKS?

When water collects in the cracks of a rock, it can freeze when temperatures drop. The ice expands and the pressure can split the rock. In cold, mountain regions, one can even hear gunshot-like cracks as rocks are split apart by frost.

A mechanical process, freeze-thaw weathering causes the joints? (cracks) in rocks to expand, which wedges parts of rocks apart. Because water expands by about 10% when it freezes, this creates outward pressure in rock joints, making the cracks larger.

Joints occur naturally in rocks as a result of their formation. Fractures that are not offset, joints do allow for the entry of water into rocks.

In climates where temperatures dip below freezing in the winter, moisture in the joints of rocks solidifies as ice. Over time, after several cycles of freezing and thawing, joints get large enough that bit of rock start to fall off in smaller pieces. This breakdown of rock happens faster at higher altitudes, where many freeze-thaw cycles can occur during the year.

Credit: Sciencing

Picture Credit : Google