Astronomers Have Found a Black Hole That's Erupting With Strange Regularity

Astronomers have found a supermassive black hole (SMBH) with an unusually regular feeding schedule.

The behemoth is an active galactic nucleus (AGN) at the heart of the Seyfert 2 galaxy GSN 069. The AGN is about 250 million light years from Earth, and contains about 400,000 times the mass of the Sun.

The team of astronomers used the ESA's XMM-Newton and NASA's Chandra X-ray Observatory to observe the x-ray emissions of the SMBH. About every 9 hours, black hole flares brightly with x-rays

Astronomers have found two other stellar mass black holes that flare regularly as they feed, but this kind of regularity in a supermassive black hole has never been seen before.

The paper outlining this discovery is published in Nature and is titled "Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus."

Lead author is Giovanni Miniutti from ESA's Center for Astrobiology in Spain.

According to the paper, the SMBH consumes about four months worth of material. That means every time the black hole feeds, it consumes about a million trillion pounds of material.

"This black hole is a meal plan like we've never seen before," said Miniutti in a press release.

"This behavior is so unprecedented that we had to coin a new expression to describe it:" X-ray Quasi-Periodic Eruptions "."

X-ray emissions from this SMBH have been known and observed since July 2010, but they are steady. The new paper is based on 54 days of observations beginning in December 2018, beginning with the ESA's XMM-Newton Observatory.

That observatory spotted two bursts on December 24th. In January, XMM-Newton found three more of these regular bursts.

Then astronomers requested more observing time with NASA 's Chandra Observatory to investigate. Chandra observed five more of these events.

During the current regular eruptions, the X-ray flaring activity increases by two orders of magnitude over the X-ray emissions. Each flare lasts just over one hour and occurs every nine hours.

Two initial flares (blue) plus subsequent flares spotted by XMM-Newton (green) and Chandra (red). (G. Miniutti and. al., 2019.)

"By combining data from these two X-ray observatories, we have tracked these periodic outbursts for at least 54 days" said co-author Richard Saxton of the European Space Astronomy Center in Madrid, Spain.

"This gives us a unique opportunity to witness the flow of a supermassive black hole repeatedly speeding up and slowing down."

During each of these outbursts, the X-ray is in full swing. The temperature of the in-fall also rises. It rises from about 1 million degrees Fahrenheit in quieter periods to 2.5 million degrees Fahrenheit during flares. The higher temperature is about the same temperature as most SMBHs that are actively growing.

The cause of these regular flares is unknown. The hot 2.5 million degree F. gas surrounding GSN 069 is the same temperature as gas surrounding other SMBHs. It's a mystery because it's just too hot to be in the background of material that surrounds black holes. Purpose GSN 069 is a unique opportunity to study the phenomenon because of the hot gas again forms then disappears.

Normally, this hot gas is caused by a star being torn apart and consumed by a black hole, or so astronomers think. But the regularity exhibited by GSN 069 is a mystery.

"We think the origin of the X-ray is a bit of a bit," said co-author Margherita Giustini, also of ESA's Center for Astrobiology.

"But as for the repeating bursts, this is a completely different story which originates in the future."

Again, see supermassive black hole consume gas from a star is nothing new. It's the regularity of GSN 069's flaring that is the head-scratcher. The authors of the study suggest two possible explanations for the SMBH's regular feeding schedule:

• The amount of energy in the form of the unstable and rapidly falling into the black hole producing the bursts. That cycle is repeating.
• There is an interaction between the disk and a secondary body orbiting the black hole, perhaps the remnant of the partially disrupted star.

Thanks to the Chandra observations, the team of scientists knows that the source of the flaring X-rays is right in the heart of GSN 069. That's where SMBH is expected to be.

The combined data from Chandra and XMM-Newton show clearly that flaring, though regular, is slowly changing and both the size and the duration of the meal are slightly increased. It's up to future observations.

GSN 069 is on the small side for an SMBH. Usually, an SMBH contains more than one million or more Suns, while GSN 069 contains only about 400,000 Suns worth of mass. That could help explain why this type of feeding.

For larger SMBHs, much larger than this one, their brightness fluctuations are a lot slower. Rather than erupting every nine hours, it should take them months or even years to flare like this. That would explain why quasi-periodic eruptions (QPEs) like these have not been observed. X-Ray observatories are busy, and there's no way to get along.

There have been several cases where large numbers of X-rays produced by black holes have been observed. Those observations are repeated over months, or even years.

Some of those changes are too much explained by the standard theory of in-falling matter from a black hole's accretion disk. But this discovery could explain those observations. They may be experiencing similar behavior as GSN 069.

This article was originally published by Universe Today. Read the original article.