What's Happening in the Milky Way's Core?

black hole in milky way core
The Center of our Milky Way as you won't see it with the naked eye. This is a radio-astronomy "image" of the central part of our galaxy. The brightest source is Sagittarius A*. The bright diagonal features trace our Galaxy’s disk-like shape viewed edge-on. The Galaxy's center lies toward the constellation Sagittarius, or Sgr.) Deep within Sgr A is Sgr A*, a black hole with a mass millions of times that of the Sun. Hot young stars heat the gas around them in bright, round blobs. Massive supernovae explosions leave bubble-shaped remnants. Spiraling or synchrotron radiation seems makes a collection of strange, thread-like structures. Their emission, orientation, and structure provide important clues about the energetics and large-scale magnetic field structure here. NRAO

Something's happening at the heart of the Milky Way galaxy. The supermassive black hole — named Sagittarius A* — which lies right at the center of our galaxy is usually quiet, for a black hole. It periodically feasts on stars or gas and dust that stray into its event horizon. But, it doesn't have strong jets as other supermassive black holes do. Instead, it's pretty quiet.

Lately it has been sending out "chatter" that's visible to x-ray telescopes.

What kind of activity would cause it to suddenly wake up and start sending out emissions? 

Alerted by the data, astronomers began looking at possible causes. Sagittarius A* seems to produce about one bright x-ray flare every ten days or so, as picked up by long-term monitoring done by the Chandra X-ray Observatory, Swift, and XMM-Newton. Then, suddenly in 2014, the black hole kicked up its messaging — producing a flare every day. 

A Close Approach Starts Sgr A* Chattering

What could have irritated the black hole? The uptick in x-ray flares happened soon after the
close approach to the black hole by a mysterious object astronomers have named G2. Astronomers long thought G2 was an extended cloud of gas and dust in motion around the central black hole. Could it be the source of material for the black hole's feeding uptick? In late 2013, it passed very close to Sagittarius A*. The close approach didn't tear apart the cloud (which was one possible prediction of what might happen).

But, the black hole's gravity did stretch the cloud a bit. 

What's Happening? 

That posed a mystery. If G2 was a cloud, it very likely would have been stretched quite a bit by the gravitational tug it experienced. It didn't. So, what could G2 be?  Some astronomers suggest it might be a star with a dusty cocoon wrapped around it.

If so, the black hole may have sucked some of that dusty cloud off, and when the material encountered the black hole's event horizon, it would have been heated enough to give off x-rays.

Another idea is that G2 has nothing to do with the black hole's emissions. Instead, there could be some other change in the region that is causing Sagittarius A* to give off more x-ray flares than usual. 

The whole mystery is giving scientists another look at how material is funneled into our galaxy's supermassive black hole and what happens to it once it gets close enough to feel the gravitational pull of Sagittarius A*. 

Black Holes and Galaxies

Black holes are ubiquitous throughout the galaxy, and supermassive ones exist at the hearts of most galactic cores. In recent years, astronomers have figured out that central supermassive black holes are an integral part of a galaxy's evolution, affecting everything from star formation to the shape of a galaxy and its activities.

Sagittarius A* is the closest supermassive black hole to us — it lies at a distance of about 26,000 light-years from the Sun. The next closest one lies at the heart of the Andromeda Galaxy, at a distance of 2.5 million light-years. These two provide astronomers with "up-close" experience with such objects and help develop an understanding of how they form and how they behave in their galaxies.