Using ESA’s Integral space observatory, astronomers discovered and watched a black hole in galaxy NGC 4845 feed on a low-mass object that strayed too close.
Astronomers have watched as a black hole woke up from a decades-long slumber to feed on a low-mass object – either a brown dwarf or a giant planet – that strayed too close. A similar feeding event, albeit on a gas cloud, will soon happen at the black hole at the center of our own Milky Way Galaxy.
The discovery in galaxy NGC 4845, 47 million light-years away, was made by ESA’s Integral space observatory, with follow-up observations from ESA’s XMM-Newton, NASA’s Swift and Japan’s MAXI X-ray monitor on the International Space Station.
Astronomers were using Integral to study a different galaxy when they noticed a bright X-ray flare coming from another location in the same wide field-of-view. Using XMM-Newton, the origin was confirmed as NGC 4845, a galaxy never before detected at high energies.
Along with Swift and MAXI, the emission was traced from its maximum in January 2011, when the galaxy brightened by a factor of a thousand, and then as it subsided over the course of the year.
“The observation was completely unexpected, from a galaxy that has been quiet for at least 20–30 years,” says Marek Nikolajuk of the University of Bialystok, Poland, lead author of the paper in Astronomy & Astrophysics.
By analyzing the characteristics of the flare, the astronomers could determine that the emission came from a halo of material around the galaxy’s central black hole as it tore apart and fed on an object of 14–30 Jupiter masses. This size range corresponds to brown dwarfs, substellar objects that are not massive enough to fuse hydrogen in their core and ignite as stars.
However, the authors note that it could have had an even lower mass, just a few times that of Jupiter, placing it in the range of gas-giant planets.
Recent studies have suggested that free-floating planetary-mass objects of this kind may occur in large numbers in galaxies, ejected from their parent solar systems by gravitational interactions.
The black hole in the center of NGC 4845 is estimated to have a mass of around 300 000 times that of our own Sun. It also likes to play with its food: the way the emission brightened and decayed shows there was a delay of 2–3 months between the object being disrupted and the heating of the debris in the vicinity of the black hole.
A strong hard X-ray flare was discovered in the galaxy NGC 4845 by INTEGRAL in January 2011. This emission corresponds to the tidal disruption of a super-Jupiter close to the giant black hole at the center of the galaxy. The disrupted material heated up before falling in the black hole, emitting at high energies.
“This is the first time where we have seen the disruption of a substellar object by a black hole,” adds co-author Roland Walter of the Observatory of Geneva, Switzerland.
“We estimate that only its external layers were eaten by the black hole, amounting to about 10% of the object’s total mass, and that a denser core has been left orbiting the black hole.”
The flaring event in NGC 4845 can be seen as a warm-up act for a similar event expected in the supermassive black hole at the center of our own Milky Way Galaxy, perhaps even this year.
While there are no brown dwarfs or planets on the menu this time, a compact cloud of gas amounting to just a few Earth masses has been seen spiraling towards the black hole and is predicted to meet its fate soon.
Along with the object seen being eaten by the black hole in NGC 4845, these events will tell astronomers more about what happens to the demise of different types of objects as they encounter black holes of varying sizes.
“Estimates are that events like these may be detectable every few years in galaxies around us, and if we spot them, Integral, along with other high-energy space observatories, will be able to watch them play out just as it did with NGC 4845,” says Christoph Winkler, ESA’s Integral project scientist.
Reference: “Tidal disruption of a super-Jupiter by a massive black hole” by M. Nikołajuk and R. Walter, 2 April 2013, Astronomy & Astrophysics.