Astronomers are uncovering a treasure trove of supermassive black holes in the universe, with estimates suggesting there could be billions, if not trillions, more still hidden away.
Researchers found these enormous black holes by using infrared light to see through thick clouds of gas and dust. This new information could help us better understand how galaxies grow and change over time.
Finding black holes is no easy task. They are incredibly dark — even light can’t escape their strong gravity. We sometimes catch a glimpse of them when they eat matter, causing the surrounding materials to heat up and glow. But many black holes don’t have this bright halo, so spotting them requires clever techniques.
Scientists think there are billions of supermassive black holes, each weighing at least 100,000 times more than our sun, scattered throughout the universe. It’s believed one sits at the center of every large galaxy. However, counting them all is nearly impossible, so astronomers conduct surveys of nearby galaxies to estimate how many are hidden in our cosmic neighborhood.
Many black holes stay hidden because they are covered by thick clouds of dust and gas. A recent study in the Astrophysical Journal suggests that about 35% of supermassive black holes might be obscured in this way. That figure has jumped from an earlier estimate of 15%, and some researchers think it could actually be as high as 50%.
Astronomers are getting better at locating these elusive giants. The gas and dust around hidden black holes still emit some light, but it’s in the infrared spectrum. In their latest study, researchers utilized data from two important instruments. The first was NASA’s Infrared Astronomical Satellite (IRAS), the first space telescope to study the infrared range back in 1983. The second tool was the Nuclear Spectroscopic Telescope Array (NuSTAR), which can detect high-energy X-rays produced by superheated matter around black holes.
By combining data from these sources, astronomers spotted hundreds of potential hidden black holes. They further validated their findings using ground-based telescopes and NuSTAR to confirm which candidates were indeed black holes. Some turned out to be galaxies bursting with star formation, but many were successfully identified as black holes.
Peter Boorman, an astrophysicist at Caltech, expressed amazement at how useful IRAS and NuSTAR were for this research, especially since IRAS has been out of operation for over 40 years. This technique might reveal not only how common these black holes are but also their role in shaping galaxies. Supermassive black holes may influence the size of galaxies by pulling in star-forming material or limiting their growth.
Your own Milky Way galaxy has a supermassive black hole at its center. Poshak Gandhi, an astrophysicist at the University of Southampton in the U.K., noted that without it, we might see a lot more stars in our night sky. This ongoing research opens up exciting possibilities for deepening our understanding of the universe and its hidden wonders.