More Mysterious G Objects Discovered Near Black Hole at Center of Milky Way

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Four more unusual objects have been spotted orbiting the supermassive black hole near the center of the Milky Way galaxy.

What are they?

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The orbits of the newly-discovered G objects are traced over this image of objects near the center of our galaxy. Image credit: Anna Ciurlo, Tuan Do/UCLA Galactic Center Group

Every major galaxy is home to a supermassive black hole, and our own Milky Way is no exception.

Astronomers recently found something unexpected near this massive object — four mysterious objects, each similar to a pair of bizarre bodies spotted in recent years in this same region of the galaxy.

Our local supermassive black hole, Sagittarius A* (Sgr A*), contains roughly four million times as much mass as the Sun.

Not far from this black hole, members of a newly-discovered class of objects is caught in a gravitational dance with the massive body.

These G objects look like gas, but behave like stars, as they complete their 100- to 1000-year-long orbits of Sgr A*.

While they appear compact most of the time, they stretch out as they come closer to the black hole near the core of our galaxy.

Mysterious G objects

The first G object was discovered in 2005, and was labeled G1.

Seven years later, a second body was found, and given the moniker G2.

The four newly-discovered objects are named G3 through G6.

While G1 and G2 have the orbits similar to each other, the newly-found bodies follow significantly different paths around the center of the Milky Way.

At the time of closest approach, G2 had a really strange signature. We had seen it before, but it didn’t look too peculiar until it got close to the black hole and became elongated, and much of its gas was torn apart,” said Andrea Ghez, professor of astrophysics at UCLA.

And continued: “It went from being a pretty innocuous object when it was far from the black hole to one that was really stretched out and distorted at its closest approach and lost its outer shell, and now it’s getting more compact again.

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A rendering of G objects being stretched by the supermassive black hole at the center of the Milky Way (center). Image credit: Jack Ciurlo/UCLA

Following the discovery of the first pair of these bodies, Ghez and her team studied the region near the center of our galaxy, including the examination of 13 years of data from the Keck Observatory on Maunakea in Hawaii.

No broad consensus has yet been reached concerning their nature: the G objects show the characteristics of gas and dust clouds but display the dynamical properties of stellar-mass objects,” researchers report in a new astronomy article.

Ghez believes these G objects were once pairs of binary stars which merged into single objects due to the extreme gravitational forces near the supermassive black hole.

Such a process would take roughly one million years to complete, research suggests.

The G2 mystery

Gas within the G2 object was significantly stretched by gravity from Sgr A*, while dust within the body did not expand toward the black hole to nearly the same degree.

This suggests a stellar-sized mass withing G2 is keeping the body largely intact.

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G objects and stars surrounding the supermassive black hole near the center of our galaxy. Image credit: Animated .gif created by The Cosmic Companion from video produced by the UCLA Galactic Center Group.

One of the things that has gotten everyone excited about the G objects is that the stuff that gets pulled off of them by tidal forces as they sweep by the central black hole must inevitably fall into the black hole.

When that happens, it might be able to produce an impressive fireworks show since the material eaten by the black hole will heat up and emit copious radiation before it disappears across the event horizon,” stated Mark Morris, UCLA professor of physics and astronomy.

What’s the hole story?

Sagittarius A* was first discovered in February 1974 by Bruce Balick and Robert L. Brown, using The National Radio Astronomy Observatory’s Green Bank 35 km radio link interferometer.

For eight years, astronomers suggested a number of names for the behemoth black hole, but it was not until 1982 that the name Sgr A*, coined by Brown, became the standard label for this body.

The asterisk in the name not only denotes “star,” it also hearkens to the nomenclature of chemistry, where atoms in an excited state are denoted with the same symbol.

The supermassive black hole near the center of our galaxy is not nearly as active as those seen in many other galaxies.

However, in 2005, Ghez and her team were able to show that Sgr A* is “feeding” more on incoming matter in recent years (as seen from Earth).

Mergers of stars may be happening in the universe more often than we thought, and likely are quite common.

Black holes may be driving binary stars to merge.

It’s possible that many of the stars we’ve been watching and not understanding may be the end product of mergers that are calm now.

We are learning how galaxies and black holes evolve. The way binary stars interact with each other and with the black hole is very different from how single stars interact with other single stars and with the black hole,” Ghez said.

More space news on Strange Sounds and Steve Quayle. [Nature, Medium]

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