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General Studies 3 >> Science & Technology

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SUPER MASSIVE BLACK HOLE

SUPERMASSIVE BLACK HOLE

 
 
1.Context
When it comes to making sense of our universe, the importance of black holes is hard to understate. Scientists know that a black hole exerts a strong gravitational pull, so much so that any object that gets closer to its centre beyond a point can never get back out. The effects of black holes on their surroundings include the release of a tremendous amount of energy. These effects are crucial to determining the structures of the galaxies they occupy and how the stars around them evolved over time
 
2.Black Hole
 
  • A Black hole is a region of space-time exhibiting gravitational acceleration so strong that nothing no particles or even electromagnetic radiation such as light can escape from it.
  • The theory of general relativity predicts that a sufficiently compact mass can deform space-time to form a Black hole. The boundary of the region from which no escape is possible is called the event horizon.
  • The concept was theorized by Albert Einstein in 1915 and the term 'black hole' was coined in the mid-1960s by American physicist John Archibald Wheeler.
Usually, black holes belong to two categories:
  • One category ranges between a few solar masses and tens of solar masses. These are thought to form when massive stars die.
  • The other category is supermassive black holes. These range from hundreds of thousands to billions of times that of the sun from the solar system to which Earth belongs.
 

3.Types of Black Holes

There are four different forms of black holes
  1. Stellar
  2. Intermediate
  3. Supermassive
  4. Miniature
  • The first is the SMBH, or supermassive black hole. This is the largest variety, with an unquantifiable number of solar masses. This is typically found at the heart of the universe's biggest galaxies. The SMBH is located in Sagittarius A in our solar system.
  • The second is the singularity, which is the black hole's eye (or core). This is the point at which the curve becomes infinite.
  • The photon sphere, a spherical boundary (with no thickness) where photons move perpendicularly to the sphere and are imprisoned in an elliptical orbit about the black hole, is the third.
  • A micro black hole, also known as a little black hole or a quantum mechanical black hole, is the last form. Stephen Hawking first mentioned them in 1971.

4.Formation of Black hole

  • Astronomers believe that depending on a star's mass, only one of the three things can happen once it runs out of fuel. A star with a mass less than that of the sun falls into a 'white dwarf' with a radius of barely a few thousand kilometres.
  • If the mass of the star is between one and four times that of the sun, it can form a 'neutron star with a radius of only a few kilometres, which is known as a 'pulsar'.
  • Only a few stars with mass greater than four times that of the sun may avoid collapsing and creating black holes within their Schwarzschild radii. As a result, black holes could be the remains of enormous stars.
  • Milky way, according to most astronomers, was born from a vast cloud of gas that collapsed and broke up into individual stars.
  • The nucleus, or core, of the galaxy, presently contains the most densely packed stars. It's possible that there was too much substance at the very centre to form a regular star, or that the stars that did form were too close together to form a black hole.
  • As a result, it's been proposed that black holes as huge as a hundred million Suns could exist in the centre of some galaxies.

5.Rare Supermassive blackhole

  • A rare supermassive black hole has been spotted by a team of Indian researchers and The monster black hole is about one billion light years away from the Earth. The black hole in question was captured, spewing a jet of radiation and particles in one direction, unlike others that fire jets in opposite directions. But strangely for this galaxy, only one side of the jet is seen. The supermassive black holes create powerful jets and radiation and particles.
  • The supermassive black hole occupies the centre of the RAD 12 galaxy, which is elliptical or egg-shaped. RAD 12 is in the process of merging with another galaxy, RAD 12b, in the next one billion years. RAD 12b, which is elliptical, is bigger and brighter than RAD 12. The jet is bigger than its host, RAD 12. It resembles a 440 thousand light-years-long mushroom.
  • This discovery may help scientists study why star formation does not occur in elliptical galaxies. Star formation requires extremely cooled gas, usually forged in a cloud of interstellar gas and dust. The temperature in these regions ranges from -253.15°C-263.15°C, according to the University of Oregon. Theoretically, jets remove cold gas and suppress star formation. Researchers speculate that jets fired by supermassive black holes will likely suppress future star formation.
 
For prelims & Mains
 
For Prelims: 
Black holes, RAD 12, RAD 12b, Supermassive black hole (SMBH), Sagittarius A
For Mains: 1. What is a Black Hole? Explain the formation and types of Black Holes. (250 words) .
 
Source: Down To Earth

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