The Bright Core of This Spiral Galaxy Reveals an Actively Feeding Supermassive Black Hole

Hubble Space Telescope observes a lot of galaxies. Some of them are wild-looking while others seem fairly placid. Recently, it looked at NGC 5495, which lies about 300 million light-years away from Earth. You wouldn’t know just by looking at it, but this galaxy has some pretty hot action happening in its core.

It’s known as a Seyfert galaxy, which means it has a very active nucleus. There’s a supermassive black hole in there, sucking in gas and dust and releasing bright radiation as it eats. Astronomers want to know more about this monster—in particular, its mass. That’s why they’re using Hubble Space Telescope to observe it. The Wide Field Camera 3 is well-suited to image the bright core and separate out the various light sources nearby so they can zero in on the region around the black hole.

Diving into a Seyfert Galaxy

Galaxies with active nuclei are fascinating places. Most look like pretty normal spirals, particularly through optical telescopes. But, if you observe them in other wavelengths—say x-rays, ultraviolet or infrared, their cores stand out like beacons. The cores are usually brighter than anything else in the galaxy. That tells you something energetic is happening there. That brightness actually is a “death scream” of sorts. Matter accretes onto the black hole and gets superheated by high-speed collisions. That maelstrom is what’s giving off light across much of the electromagnetic spectrum. About 10 percent of all galaxies are Seyferts and they were probably quasars earlier in their histories.

Here’s another Seyfert galaxy as seen by Hubble. It’s called Messier 77. The streaks of red and blue in the image are star formation regions in the arms, with dark dust lanes stretching across the galaxy’s starry centre. This Seyfert has highly ionised gas surrounding an intensely active center. Courtesy NASA/ESA/STScI.

Astronomers classify Seyferts into Type 1 and Type II objects. If you look at their emission lines (that is, the spectra that show the light they emit), the data show that each kind has highly excited gas near the black hole. There are important differences though. The Type 1 Seyferts have very “broad” lines, which means that the gas is moving very quickly around the black hole—at velocities more than 1,000 km/sec. On the other hand, the Type II Seyferts have narrower lines, and that means gas in the core is moving much more slowly.

Our own Milky Way is not currently a Seyfert. However, it does have a central supermassive black hole called Sagittarius A*. Right now, it’s very quiet, only occasionally gobbling large amounts of gas and dust. It could have been a Seyfert in the past, or it could be in the future if something happens to feed our black hole and cause it to “erupt” with activity.

What HST Tells Us About NGC 5495

In the HST image of this spiral its arms have bands of dust threaded throughout, and there are star birth regions here and there. Notice the strands of blue in the arms. Those mainly hot young stars emit a lot of ultraviolet light. The most massive of these stars will explode as supernovae ten million or so years from now.

The core of the galaxy looks like there’s a bar feeding material into the core. In many spiral galaxies, the bars host stellar nurseries. Astronomers are quite interested in these bars because they indicate something about the age and evolutionary state of the galaxy itself. Interestingly, central bars may come and go every couple of billion years.

And, then there’s that bright central region, where the monster black hole lives and feeds. It’s likely quite massive—millions or billions of times the mass of our Sun. Sucn objects influence the evolution of their galaxies, and astronomers are still working to understand how that works. Of course, in addition to studying distant Seyfert galaxies like NGC 5495, they also look at the one in our own galaxy. Even though it’s relatively quiet today, it still acts like the others do—eating up whatever gets trapped in its strong gravitational pull.

For More Information

Hubble spies a stately spiral galaxy

Overview of Seyfert Galaxies

Carolyn Collins Petersen

Recent Posts

Colliding Neutron Stars can Generate Long Gamma-ray Bursts

Gamma-Ray Bursts (GRBs) are the most energetic recurring events in the Universe. Only the Big…

4 hours ago

“Early Dark Energy” Could Explain the Crisis in Cosmology

A new study considers how the presence of Early Dark Energy could help resolve one…

5 hours ago

How Artificial Intelligence Can Find the Source of Gamma-Ray Bursts

Gamma-ray bursts come in two main flavors, short and long. While astronomers believe that they…

6 hours ago

The Geminids Will be Peaking on December 14th. They’re Usually the Most Active Meteor Shower Every Year

Meteor showers are a great way to share a love of astronomy with those who…

8 hours ago

A Star was Blocking a Galaxy, but Now it’s Moved Enough That Astronomers can Finally Examine What it Was Hiding

One of the biggest puzzles in astronomy, and one of the hardest ones to solve,…

9 hours ago

Will We Ever Go Back to Explore the Ice Giants? Yes, If We Keep the Missions Simple and Affordable

It's been over 35 years since a spacecraft visited Uranus and Neptune. That was Voyager…

1 day ago