Image from Hubble Space Telescope shows an Intriguing 'Active' Galaxy
An active galactic nucleus (AGN) is a small area at the centre of some galaxies that is much brighter than the galaxy's stars alone would be.
- Science News
- 3 min read

Z 229-15, a celestial object in the constellation Lyra, is visible in the bright image taken by the NASA/ESA Hubble Space Telescope. It is placed about 390 million light-years away from Earth. One of those intriguing celestial objects, Z 229-15 has been classified as an active galactic nucleus (AGN), a quasar, and a Seyfert galaxy at various points in time as per reports from NASA.
Which of these actually contains Z 229-15?
The answer is that it is all of these things at once since there is a large overlap between these three definitions.
An active galactic nucleus (AGN) is a small area at the centre of some galaxies that is much brighter than the galaxy's stars alone would be. The supermassive black hole that is located at the galaxy's centre is the cause of the increased luminosity. Instead of falling directly into a black hole, the material is attracted into a spinning disc and then is irresistibly pulled in that direction.
AGNs are so bright because of the enormous amount of energy that is released across the electromagnetic spectrum when this disc of stuff becomes extremely hot.
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Quasars are a specific kind of AGN; they are often very bright and very far away from Earth. Z 229-15 is positively local since it is located inside a quasar's range of proximity, which is several hundred million light-years. Yet, Seyfert galaxies are active galaxies that house extremely bright AGNs (quasars) while the remainder of the galaxy is still viewable.
Frequently, an AGN is so luminous that the rest of the galaxy cannot be observed. Z 229-15 is a Seyfert galaxy that, by definition, hosts an AGN because it contains a quasar.
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