P172+18 Quasar

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  • An international team of astronomers have discovered the most distant ‘radio-loud’ quasar with the help of the European Southern Observatory’s Very Large Telescope (ESO’s VLT).

About the Discovery

  • It is named P172+18, the quasar emitted wavelengths which had a redshift of 6.8.
    • Gravitational redshift occurs as particles of light (photons) climb out of a gravitational well like a black hole and the light’s wavelength gets drawn out. This shifts the wavelength to the red part of the light spectrum – hence “redshift”.
    • It took 13 billion years for the quasar’s light to reach earth.
    • The higher the redshift of the radio wavelength, the farther away is the source.
  • The glowing disc around a blackhole is 300 million times more massive than our Sun.
  • It is also one of the fastest accreting quasars, which means it is accumulating objects from the galaxy at an enormous speed.
  • Only three other ‘radio-loud’ sources with redshift greater than six have been discovered so far and the most distant one had a redshift of 6.18.
  • The scientists think that the powerful radio jets shooting out of the quasar fuelled the appetite of the black hole.
    • The jets are thought to be capable of disturbing the gas around the black hole, increasing the rate at which gas falls in.
  • Inference: The blackhole at its centre is consuming from its galaxy at a stunning rate.

Significance

  • A detailed study of these ‘radio-loud’ super bright objects can help the astronomers to understand how the supermassive black holes in their core grew to be as big so rapidly since the Big Bang.
  • The team believes that more such quasars that tell stories about the ancient universe will be found, perhaps even farther away from earth.

What are Quasars?

  • Quasi Stellar radio sources, abbreviated QUASARS, are the most dynamic and far-off objects in a collective known as active galactic nuclei (AGN).
  • Its spectrum consisted of wide emission lines, unlike stars, thus the name “quasi-stellar.”
  • These radiant sources were formed approximately twelve billion years ago.
  • Quasar formations take place by the collision of galaxies, i.e., the central black holes merge to form a supermassive black hole.
  • Quasars are very luminous objects in faraway galaxies that emit jets at radio frequencies. They are only found in galaxies that have supermassive black holes which power these bright discs.
  •  However, 90 percent of them do not emit strong radio waves, making this newly-discovered one special.
  • Most active galaxies have a supermassive black hole at the centre which sucks in surrounding objects.
  • Although quasars were originally discovered due to their radio emissions, only about 10% of quasars have substantial radio emissions.
    • These quasars are now called radio-loud quasars.
    • Quasars without strong radio emissions are called radio-quiet quasars

Blackhole

  • It is a region in space where the pulling force of gravity is so strong that neither matter nor light can escape. This phenomenon occurs when a star is dying.
  • For anything approaching a black hole, the point of no return is called the “event horizon” and anything that comes within the event horizon will be consumed forever.
  • Since no light can escape from it, a black hole is invisible.
  • However, advanced space telescopes can identify black holes by observing the behaviour of material and stars that are very close to black holes.
  • This hot disk of material encircling a black hole shines bright and against this disk, a black hole appears to cast a shadow.
  • This is how the photograph of the black hole was achieved.
  • In 2019, NASA released the first-ever photograph of a black hole and its shadow, which was captured by an international network of radio telescopes called the Event Horizon Telescope (EHT).
    • The image shows the shadow of a supermassive black hole in the centre of Messier 87 (M87), an elliptical galaxy some 55 million light-years from Earth.
    • This black hole is 6.5 billion times the mass of the Sun.

About the ESO’s VLT:

  • The Very Large Telescope array (VLT) is the flagship facility for European ground-based astronomy at the beginning of the third Millennium.
  • Very Large Telescope (VLT), an observatory located on the mountain Cerro Paranal (2,635 metres [8,645 feet]) in Chile
  • It is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter and four movable 1.8m diameter Auxiliary Telescopes.
    • The telescopes can work together, to form a giant ‘interferometer’.
  • The ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes.

Source :DTH

 
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