Here’s What Happens When a Supermassive Black Hole Fails to Do Its Job [Video]
- A new study reveals what happens when a supermassive black hole in the center of a galaxy cluster stops being active.
- By combining data from Chandra, Hubble, and Spitzer data, astronomers found a deluge of star formation in the cluster known as SpARCS1049.
- SpARCS1049 is producing stars at a rate some 300 times that seen in the Milky Way galaxy.
- This result is in contrast with many other clusters that show how active supermassive black holes keep gas too hot to form many stars.
A galaxy cluster is demonstrating what can happen when a supermassive black hole stops being active. SpARCS104922.6+564032.5 (SpARCS1049 for short) is a galaxy cluster located 9.9 billion light years away from Earth. Galaxy clusters contain hundreds or thousands of galaxies pervaded by hot, X-ray emitting gas that outweighs the combined mass of all the galaxies. In this image of SpARCS1049, X-rays from NASA’s Chandra X-ray Observatory (light blue) have been combined with optical and infrared light data from NASA’s Hubble Space Telescope (red, green, and blue).
Astronomers have seen many examples where a supermassive black hole in a cluster’s central galaxy prevents this hot gas from cooling to form vast numbers of stars. This heating allows supermassive black holes to influence or control the activity and evolution of their host cluster.
However, the would-be domineering black hole in SpARCS1049 is behaving differently and is almost completely dormant. This appears to be allowing star formation to run rampant. According to observations from Hubble and NASA’s Spitzer Space Telescope, SpARCS1049 is forming stars at a rate over 300 times our Milky Way galaxy. (At this rate of SpARCS1049, all of the stars in the Milky Way could form in just 100 million years, which is one percent of our Galaxy’s age of more than 10 billion years.)
Researchers tried to determine what is causing this explosion of star formation and why it is located about 80,000 light years away from the center of SpARCS1049, outside any of the cluster’s galaxies. The Chandra data show that the temperature of the gas in the site of prodigious star formation has cooled to about 10 million degrees. (This is in contrast to most of the rest of the cluster where the gas is hotter at about 65 million degrees.) The presence of this cooler gas suggests that other undetected gas reservoirs have cooled to even lower temperatures that enable huge numbers of stars to form.
An annotated version of the composite image shows the location of the densest hot gas seen with Chandra, along with the galaxy in the center of the cluster. The coolest gas detected by Chandra and the site of the most rapid star formation is located halfway between the densest gas and the central galaxy.