A Titanic Supermassive Black Hole Residing in a Galactic Backwater

Makes astronomers think they need to rethink theory on black hole formation 

Scientists generated this computer simulation showing a supermassive black hole lurking at the center of a massive galaxy. The black sphere seen here at the core of the galaxy is its event horizon, beyond which not even light can escape the gravitational grip of this monster. A gravitational force that distorts spacetime near it and stretches and smears light from background stars as it travels past the black hole. Image credit: NASA/STSci/ESA

Space news (Black hole formation theory) – 200 million light-years from Earth in the direction of the constellation Eridanus –

Astronomers working on current black hole formation theory have detected a supermassive black hole at the center of a galaxy in a region of space and time they didn’t expect to find such a monster. A very hungry monster containing the mass of over 17 billion suns, residing in an out-of-the-way galactic backwater town.
Previously, astronomers detected titanic supermassive black holes at the center of huge, very massive galaxies in parts of space and time with a greater density of large galaxies. The very crowded Coma galaxy cluster has over 1,000 galaxies and is home to the biggest monster supermassive black hole recorded with an estimated mass of 21 billion times that of Sol.

NGC 1600 is a massive, isolated elliptical galaxy with one of the biggest recorded monster residing at its core. A supermassive black hole estimated to contain the matter found within 17 million suns like our own. Credit: NASA, ESA, Digital Sky Survey 2

“The newly discovered supersized black hole resides in the center of a massive elliptical galaxy, NGC 1600, located in a cosmic backwater, a small grouping of 20 or so galaxies,” said lead discoverer Chung-Pei Ma, a University of California-Berkeley astronomer and head of the MASSIVE Survey, a study of the most massive galaxies and supermassive black holes in the local universe. “While finding a gigantic black hole in a massive galaxy in a crowded area of the universe is to be expected – like running across a skyscraper in Manhattan – it seemed less likely they could be found in the universe’s small towns.”
“There are quite a few galaxies the size of NGC 1600 that reside in average-size galaxy groups,” Ma said. “We estimate that these smaller groups are about 50 times more abundant than spectacular galaxy clusters like the Coma cluster. So the question now is, ‘Is this the tip of an iceberg?’ Maybe there are more monster black holes out there that don’t live in a skyscraper in Manhattan, but in a tall building somewhere in the Midwestern plains.”

Ground-based view of NGC 1600
This is an image of lonely, wandering NGC 1600 taken by ground-based telescopes. Credit: NASA/ESA/Digitized Sky Survey 2

Astrophysicists studying NGC 1600 detected a supermassive black hole at least ten times more massive than current theory predicted at its center. Scientists previously thought the more massive the central bulge of a galaxy, proportionally more massive the supermassive black hole at its center should be, but this throws a wrench in previous correlations between the mass of a supermassive black hole and its central bulge of suns.

“It appears that that relation does not work very well with extremely massive black holes; they are a larger fraction of the host galaxy’s mass,” Ma said.

What could cause this smaller galaxy in a cosmic backwater to have such a titanic supermassive black hole at its core? It could be NGC 1600 merged with another galaxy hundreds of millions of years ago when such collisions were more common in this region of spacetime. Computer simulations show the central supermassive black holes of two merging galaxies fall into the center of the recently formed galaxy and begin orbiting each other in a slowly diminishing radius. Stars and other stellar objects that fall into the core steal momentum from the twirling monsters and in the process are often flung from the center of the galaxy. This transfer of momentum causes the supermassive black holes to slowly move closer together and eventually merge to form a super monster. A super monster that continues to grow by devouring gas drawn into the center of the galaxy by collisions and gravity.

In the words of Ma, “To become this massive, the black hole would have had a very voracious phase during which it devoured lots of gas.”

Astronomers continue to watch

Is it possible constant merging of NGC 1600 with galactic neighbors is one reason it lives in a cosmic backwater, with relatively few nearby galactic neighbors? It’s the brightest galaxy in town, more than three times brighter than any member of its galactic group. This difference in brightness has rarely been observed in other galactic groups. Maybe lots of galactic mergers resulted in one of the most titanic supermassive black holes ever recorded, residing in a small, cosmic backwater town.

The super monster lurking at the center of NGC 1600 is currently sleeping, but astronomers are watching for signs of its next meal going down. While they wait, they’re working on updating current theory on the formation of black holes, using the data obtained by studying NGC 1600 and similar galaxies. Current theory that will likely need to be revamped once new data comes in during our journey to the beginning of space and time.

The tide of science may rise and fall, but it always seeks truth in the facts. 

Take the space journey of NASA here.

Learn more about NGC 1600.

Learn more about supermassive black holes here.

Read more about black hole formation theory.

Learn more about the things astronomers learn by looking at the light from distant, young stars.

Supermassive black holes engulf any mass coming to close, and often burp after a meal.

Read about the weird light signal given off by two black holes that are destined to merge.

Star Light, Star Bright

Supernova SN 2005E Says Hello to the Universe

Astronomy allows you to witness some of the biggest explosions in the universe
Supernova SN 2005E shines brightly on the edge of spiral galaxy NGC 1032

 An explosion for all time

Astronomy News – A supernova is one of the most spectacular and massive events astronomers journeying backward to the beginning of space and time view, and can often be billions of times as bright as Sol, or shine brighter than an entire galaxy. Take a journey to a supernova, like SN 2005E, which astronomers became aware of when it lite up the spiral galaxy NGC 1032 in 2005, and your view of life and the universe would change forever.

Supernova SN 2005E is shown in the halo of NGC 1032 (red arrow)

Astronomers spend countless hours looking for new supernovae to study

Astronomers had previously only viewed supernovae occurring in two ways during their Journey to the Beginning of Space and Time. In the first example, the massive core of a star collapses inward near the end of its life cycle, creating a shock wave that expels the star’s outer layers into the cold darkness of space and time. In the second, a white dwarf star steals matter from a companion star, until it reaches 1.4 solar masses. At this point, the white dwarf star is unable to support more mass, according to natural law, and detonates in a titanic stellar explosion brighter than a galaxy.

A team of astronomers looking at the data obtained by space scientists studying supernova SN 2005E believe this supernova could represent a third as yet unseen, path nature uses to create a supernova. This analysis of this team of scientists has determined that this supernova occurred in a region of space and time devoid of massive stars. They also determined that this supernova only ejected a small volume of stellar material (0.3 solar masses) and abnormally high levels of calcium and radioactive titanium into the universe.

Team member Alex Filipenko of the University of California, Berkeley, and team leaders Hagai Perets of the Harvard-Smithsonian Center for Astrophysics in Cambridge and Avishay Gal-Yam of the Weizmann Institute of Science in Rehovot, Israel, conclude supernova SN 2005E took place between a low-mass white dwarf star that was stealing helium from a companion star. They also believe the volume of calcium released during supernova SN 2005E was large enough that only a few similar supernovae would be sufficient per century to provide all of the calcium presently viewed in the Milky Way Galaxy.

Supernova SN 2005E Says Hello to the Universe

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