About 61 years ago, while analysing the spectrum of a distant star, the Dutch-born American astronomer Maarten Schmidt saw unusual lines, brightness, and glitter recorded by American astronomical observatories.
The scientist reviewed the data he obtained, thinking his eyes were fooling him. The ambiguous lines, however, remained the same.
Schmidt sent several letters to other observatories to confirm the data, only to realise months later that he had discovered something completely new.
One year later, in 1964, the Taiwanese-born American scientist Hong-Yee Chiu coined a term to describe the distant and luminous objects Schmidt discovered. The term now widely known for pseudo-stars is “quasars”.
This groundbreaking discovery revolutionised our understanding of the universe by revealing the presence of incredibly distant and luminous objects supported by supermassive black holes.
Since their discovery, quasars have been the subject of extensive studies about different wavelengths of light. This has contributed significantly to our knowledge of cosmology, galaxies, and the physics of black holes.
According to the journal Nature, astronomers believe they may have found the brightest object in the universe. The quasar draws its energy from a black hole that grows so fast that it swallows the equivalent of the sun's mass every day.
The quasar's accretion disk, which scientists call J0529-4351, emits light 500 trillion times stronger than sunlight.
The data show that the black hole that feeds that distant quasar is 15 to 20 billion times the sun's mass and is about 12 billion light-years away from Earth.
What are quasars?
A quasar is an astrophysical phenomenon characterised by the presence of a stunningly luminous and active object in the centres of distant galaxies, supported by the accumulation of matter onto a supermassive black hole.
These objects emit radiation across the electromagnetic spectrum, from radio waves to X-rays and gamma rays, with a luminosity beyond the brightness of entire galaxies.
They are thought to represent an active stage in the evolution of galaxies, where the gravitational energy of the incident matter generates intense heat and radiation, creating a bright star-like appearance.
Christian Wolf, an astronomy researcher at the Australian National University, who’s the lead author of the study, says that the quasar itself is a “fast-growing black hole".
Speaking to Al Majalla, he says what makes the black hole visible to scientists “is the growth that devours everything around it.”
If a black hole stops growing, “it’s impossible to see it because it doesn’t reflect light at all". But when the black hole grows, the matter that it devours is sucked in.
The phenomenon is called the accretion disk, which is “a pattern of cohesion in which matter rotates around the black hole closer to it until it’s swallowed by it.”
As the material rotates, a great amount of heat is produced, making black holes “shine brighter than galaxies. That brilliance appears in quasars, Wolf said.