Category Science

What are some interesting facts about tigers?

Meet the animal whose tongue is hard and rough enough to tear off one’s skin to the bones.

Tigers

The tiger’s tongue is covered with numerous small, sharp, rear-facing projections called papillae. These papillae give the tongue its rough, rasping texture and is designed to help strip feathers, fur and meat from prey. The tongue can lick the paint off a wall!.

  • A tiger’s intimidating roar has the power to “paralyze” the animal that hears it and that even includes experienced human trainers. Their distinguished roar results from their extremely thick and well developed vocal cords.
  • Tigers have furs and stripes as designs on their bodies. These stripes are deep into their skin as they can still be seen after the fur is shaved

No two tigers have the same stripes. Like human fingerprints, their stripe patterns are unique to each individual.

 

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An asteroid impact is believed to have contributed to the extinction of the dinosaurs. When did this happen?

The dinosaur-killing crash threw huge amounts of debris into the air and caused massive tidal waves to wash over parts of the American continents. There is also evidence of substantial fires from that point in history.

For a long time it was thought that the non-bird dinosaurs died out 65 million years ago.

But Paul explains, ‘The dating of those layers of clay around the world is very accurate – it’s estimated to within a couple of thousands of years.

As originally proposed in 1980 by a team of scientists led by Luis Alvarez and his son Walter, it is now generally thought that the K–Pg extinction was caused by the impact of a massive comet or asteroid 10 to 15 km (6 to 9 mi) wide, 66 million years ago, which devastated the global environment, mainly through a lingering impact winter which halted photosynthesis in plants and plankton.

The blame can’t solely rest on the asteroid. Prior to its crash landing, Earth was experiencing a period of climate change. This was making things harder for life on our planet.

In what is now central India, there was substantial volcanic activity that, although unrelated to the asteroid impact, was causing problems of its own. The resulting lava outcrop is now known as the Deccan Traps.

Paul says, ‘For two million years there was a huge amount of volcanic activity going on, spewing gases into the atmosphere and having a major impact on global climate.

 

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What is the purpose of Rudram-1 missile?

RudraM-1 is India’s first indigenous anti-radiation missile. It was successfully flight tested on October 9 by the Defence Research and Development Organisation (DRDO), which developed it. Once it is ready for induction. RudraM-1 will part of the tactical weaponry of the Indian Air Force. The new generation anti-radiation missile with a speed of Mach 2 (twice the speed of sound) is likely to be integrated into the IAFS Sukhoi fighter jets.

Purpose of an anti-radiation missile

An anti-radiation missile is a missile designed for use against enemy radars on the ground. Besides detecting these missiles can target radiation-emission sources, jammers (devices used to disrupt signals from reaching) and radios used for communication and Surveillance. Mainly used in the initial part of an air conflict to strike at the air defence systems of the enemy, they can play a crucial role in disrupting jamming platforms and destroying radars, thereby clearing the way for fighter jets to launch attacks. It is also said that the missiles can prevent own systems from getting jammed.

Bang on target

According to the DRDO, RudraM-1, launched from a Su-30 MKI fighter jet, hit the radiation target located on the Wheeler Island off the coast of Odisha with pinpoint accuracy. The target seeking air-to-surface missile has a strike range of 250 km and can be launched from heights of 500 metres to 15 km.

Its navigation mechanism comprises an Inertial Navigation System (a computerised mechanism) and a Global Positioning System, which is satellite-based. Armed with a guidance system called Passive Homing Head, which can detect, classify and engage targets, RudraM-1 can detect radio emissions 100 km away. Once the missile locks onto the radiation target it is capable of hitting it accurately even if the enemy switches off the radar midway.

 

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How heavy objects sent to space?

Every year the world sends satellites and spacecraft to space to improve communications on Earth or to explore planets and moons. But how are these heavy objects sent to space?

A rocket ride

We launch things into space by putting them onto rockets that carry tonnes of propellants (fuel). These propellants give the rocket enough energy to boost away from Earth’s surface. Because of Earth’s gravitational pull the heaviest and the largest satellites or spacecraft need the biggest of rockets with most propellant.

Action and reaction

We now know that we need a rocket to send objects to space, but how does a rocket lift off? The most important idea behind a rocket’s lift off is Issac Newton’s over 300-year-old law, which states that for every action there is an equal and opposite reaction.

If you have seen photos and videos of a rocket launch, you would not have missed seeing exhaust streaming from the bottom of the rocket. This exhaust is the flames, hot gases and smoke that come from burning the rockets propellants. This exhaust pushes out from a rocket’s engine down toward the ground. This is the action force. In response to this action, the rocket begins moving in the opposite direction, lifting off the ground. This is the reaction force.

Let’s keep moving

While the rocket will lift off due to the reactive force of the exhaust, Earth’s gravity will continue pulling it down. So how does the rocket continue moving upwards? When a rocket bums propellants and pushes out exhaust an upward force called thrust is created. To launch, the rocket needs enough propellants to create thrust that is greater than the force of the gravity pulling the rocket down. A rocket needs to speed up to at least 29,000 km/hr and fly above most of the atmosphere in a curved path around Earth. This will ensure that the gravity will not pull it back down.

 

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What is the mystery of centaurs?

Is it an asteroid? Is it a planet? Is it a comet? If there is a solar system object that neither gives a resounding yes nor a certain no to these questions, then chances are that they belong to a class of celestial objects called centaurs. While estimates for the number of centaurs in the solar system are now placed anywhere above 44,000, they still remain mysterious with secrets to be revealed.

Despite their current count being in the thousands, we have been aware of their existence for less than half-a-century. And it all started in 1977, when Chiron, the first-identified member in what was then a new class of objects, was discovered.

Blink and you miss it

American astronomer Charles Kowal, who had already discovered one of the moons of Jupiter, was searching for peculiar objects in the solar system. Working at the Hale Observatories in California, the U.S., Kowal photographed the skies with telescopes and then examined them on a blink comparator – the device that had enabled American astronomer Clyde Tombaugh to discover Pluto in 1930.

The blink comparator holds two photographic plates and alternates them rapidly. While stars, which are fixed, remain steady as the plates alternate, any moving object – be it a comet, planet or asteroid – appears to jump from one plate to another. Using photographic plates of the sky in the constellation Aries on October 18 and 19, 1977, Kowal was able to discover Chiron on November 1.

How to classify

While media organisations were ready to call it the most distant asteroid discovered or even the 10th planet (Pluto was still classified as a planet in 1977), the astronomers realised that they had a question in their hands as classification wasn’t proving to be straightforward. It eventually became the first centaur, named after the half-human, half-horse being in Greek mythology, a new class of objects.

Chiron was named after the centaur Chiron in Greek mythology, believed to be the wisest and most just among all centaurs. The names of other centaurs in mythology were to be reserved for other objects that were to fall into this type.

The first centaur to be discovered, in fact, was 944 Hidalgo in 1920. It wasn’t until 2060 Chiron was discovered that astronomers realised that these belonged to a distinct group unlike any other in the solar system. Chiron, too, has been identified in images going back to 1895 following its discovery, which enabled us to determine its orbit more accurately.

Many things at once

Centaurs are now known to be a little bit of everything – asteroids, planets and comets. Small solar system bodies orbiting the sun between the outer planets, they usually have unstable orbits and are too small to be observed. Most centaurs inhabit the complex, dynamic region between Jupiter and Neptune.

Observations of 10199 Chariklo, the largest confirmed centaur so far, have revealed that it has a system of rings, akin to the ones popularly associated with Saturn, and also seen with Jupiter, Uranus and Neptune. There is a possibility that Chiron too has rings like Chariklo.

While the rings enable centaurs to draw parallels with planets, their colour and composition gives them a different identity. Most of them are either reddish or blue to blue gray in colour. We now know that the blue and blue gray centaurs are dark objects like comets and ones that are red are more like asteroids, having an organic surface.

Blue centaurs are composed of ice and are covered by a layer of dust, much like comets. This, along with highly elliptical orbits, suggests that some centaurs either are, or could become, comets.

Astronomers and astronomical organisations worldwide are involved in both classifying and cataloguing centaurs, whose numbers have been ever-increasing since they were identified to be a separate class of objects. These centaurs, like their namesake, are for now seen to be many things at the same time. They might, however, well be holding clues to some of the questions regarding our solar system for which we are still searching for answers.

 

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Why is Bennu being studied?

Over 200 million miles away from Earth, a spacecraft called OSIRIS REX studying the asteroid Bennu reached out its robotic arm to carry out a touch and go (TAG) manoeuvre at the site called Nightingale” to collect a sample from the asteroids surface on October 20. The one foot-wide sampling head made contact with Bennu’s surface for approximately 6 seconds, after which the spacecraft performed a back away bum. The sample will be returned to Earth in 2023.

What’s OSIRIS-REX mission all about?

NASA launched the sample-return mission OSIRIS REX (Origins, Spectral Interpretation, Resource Identification Security. Regolith Explorer) to the near Earth asteroid Bennu (officially 101955 Bennu) in 2016, OSIRIS-REX reached the proximity of Bennu in December 2018. It spent the next several months collecting and sending back data and images to help the NASA team on Earth learn more about the asteroid’s composition. In August 2019, NASA selected four candidate sample sites, namely Nightingale, Kingfisher, Osprey, and Sandpiper. In December 2019, Nightingale was confirmed to be the spot to carry out the mission’s primary goal of collecting sample from the asteroid’s surface.

What are the other objectives of the mission?

1) Mapping the asteroid

2) Documenting the sample site

 3) Measuring the orbit deviation caused by non-gravitational forces and

4) Comparing observations at the asteroid to ground-based observations.

What do we know about Bennu?

  • Bennu is a near-Earth asteroid, discovered in 1999.
  • It is as tall as the Empire State Building and located at a distance of about 200 million miles away from Earth.
  • It is a potentially hazardous object. It has one in 2,700 chances of impacting Earth between 2175 and 2199.
  • It is named after Bennu, an ancient Egyptian mythological bird,
  • Bennu is a “rubble pile” asteroid, which is a grouping of rocks held together by gravity.
  • Bennu completes an orbit around the Sun every 436.604 days and comes very dose to Earth every six years.
  • Bennu contains carbonaceous material which hints at the presence of water sometime in its mysterious past.
  • With the help of OSIRIS-REX, it was found that Bennu was ejecting material from its surface. Some of which fell back down, and some of which seemed to enter stable orbit.

How can the sample from Bennu help us understand the solar system better?

Scientists chose Bennu as the target of the OSIRIS REX mission because of its composition size, and proximity to Earth.

  • Bennu is classified as a B-tube asteroid which means it contains a lot of carbon and minerals. Bennu is a primitive asteroid that has not significantly changed since formation. Scientists have calculated that it might have formed in the first 10 million years of our solar system’s history over 4.5 billion years ago. Because of this, scientists hope to find organic molecules on Bennu like those that may have led to the origin of life on Earth
  • By studying Bennu, we can get a clearer picture about the formation of solar system.
  • Knowledge of Bennu’s physical properties will be critical for developing an asteroid impact avoidance mission in the future.

What next?

When going to press, NASA had not confirmed whether the arm had successfully collected sample from the surface following the touchdown. The goal was to collect at least 60 grams of sample from the surface.

If it has collected the spacecraft will prepare for its departure from Bennu in March 2021 – this is the next time Bennu will be properly aligned with Earth for the most fuel efficient return flight.

If it had failed to collect enough sample at Nightingale, then two more sampling attempts will be made. The next attempt will take place at the backup site called Osprey, which is another relatively boulder-free area inside a crater near Bennu’s equator, on Jan. 12. 2021. Whatever the case may be, the sample will be returned to Earth in 2023,

What are the other asteroid sample return missions?

OSIRIS-REX is the first asteroid sample return mission for NASA. But Japan has launched two such missions. It launched Hayabusa probe in 2003 to collect material from an asteroid called Itokawa. Things didn’t go entirely as planned, but Hayabusa did succeed in getting some tiny Itokawa grains to Earth in 2010

In December 2014, Japan launched Hayabusa 2, which collected sample in February 2019 and is scheduled to retum to Earth in December 2020.

 

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