Quasars (AQA A Level Physics)
Revision Note
Quasars
Quasars, or quasi-stellar objects, are
Extremely luminous star-like sources of radiation with very high redshifts
Quasars were first discovered in the 1960s due to their strong radio emissions but were also notable for their
High luminosities
Extremely large redshifts
Small size
Formation of Quasars
After the discovery of supermassive black holes at the centres of galaxies, astronomers were able to determine that quasars are a type of active galactic nucleus, meaning
They are supermassive black holes surrounded by an accretion disc of matter
They are found at the centre of extremely distant galaxies
When they become active, i.e. when matter falls into it, they become quasars
Structure of a Quasar
The quasar features a black hole surrounded by an accretion disk and emits jets of radiation
As matter falls into the black hole, jets of radiation are emitted from the poles
The equivalent of 100 solar masses of matter can fall into a quasar each year
The gravitational potential energy of infalling matter is transferred to electromagnetic radiation
Now it is known that quasars are strong emitters of all wavelengths, not just radio waves
Redshift of Quasars
Quasars are thought to be some of the most distant measurable objects in the known universe
This is evidenced by the extremely large redshifts they show
This allows astronomers to see very far back to an early Universe as it was not long after the Big Bang
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