Active Galactic Nucleus
An active galactic nucleus, or AGN, is an extremely bright central region of a galaxy that is dominated by the light emitted by dust and gas as it falls into a black hole.
An active galactic nucleus (AGN) is a small region at the centre of some galaxies that is far brighter than can be explained by the stellar population alone. The extremely luminous central region is emitting so much radiation that it can outshine the rest of the galaxy altogether. AGNs emit radiation across the entire electromagnetic spectrum, from radio waves to gamma rays. This radiation is produced by the action of a central supermassive black hole that is devouring material that gets too close to it. A galaxy hosting an AGN is called an ‘active galaxy’.
AGNs are the most luminous persistent sources of electromagnetic radiation in the Universe. This means they can be used to discover distant objects. Astronomers have also classified different types of AGN based on their observed characteristics. The most powerful AGNs are known as quasars, which give rise to extremely luminous galactic centres. A blazar is an AGN with a jet of light and energy that is pointed toward the Earth.
Over the years, Hubble’s instruments have observed various AGNs, including quasars. In 1996 Hubble’s 100 000th exposure was a quasar located 9 billion light-years from Earth. Hubble has also discovered the brightest quasar ever seen in the early Universe.
In 2011 Hubble captured an image of the AGN at the heart of the galaxy Markarian 509, 500 million light-years away. The AGN of this galaxy was chosen for study because it is known to vary in brightness, which indicates that the flow of matter is turbulent. Hubble’s studies of AGNs have also provided insight into how supermassive black holes interact with their host galaxies.
Additional Hubble contributions and observations can be explored by learning more about Hubble’s work in the study of quasars.