Category Archives: astronomy news

Black Holes: They’re Everywhere!

Cosmic Zombies

This image shows the location of black hole candidates found around the central region of the Andromeda Galaxy (M31). Most are stellar-mass black holes, while the central black holes in M31 are supermassive behemoths. Courtesy NASA/Chandra/

I like to read about black holes. I like to write about them, too—they’re fascinating. When I was a kid, black holes were one of those “weird cosmic things” that we’d read about in science fiction. In scientific circles, people considered them a theoretical possibility, but nobody had actually observed one. Turns out you really don’t observe a black hole. You look for the effect of the black hole on material (or space) around it. A black hole’s gravity  warps space/time, which causes light to “bend” as it travels past, sort of like looking at a straw in a glass of water. That same gravity also sucks in nearby material, which coalesces into a wide disk of material called an “accretion disk”.  The “stuff” in the disk gets funneled into the black hole, and on the way in it gets superheated. The highly hot material gives off radiation, and astronomers can spot THAT around the area of the black hole.

The black hole itself is a tightly compacted bundle of materials packed together so well and has a gravity so strong that  nothing that gets inside it—not even light—can escape it. That’s the part about black holes I think fascinates us. What’s it LIKE in there? Nobody who goes in can ever tell you because they, and their messages, would never get out.

Black holes are a continuing source of study for astronomers. They find them all over the place, scattered throughout our galaxy. Most of them are stellar black holes, meaning they were created when old, massive stars died. However, at the center of our galaxy, there is at least one (and probably two) supermassive black holes.

It turns out that other galaxies have black holes. That makes sense. They have stars, including massive ones,l so when those stars die, depending on their masses, they too will make black holes. And, the centers of other galaxies have supermassive black holes, too. Astronomers are still figuring out how those behemoth black holes get into the central regions during a galaxy’s evolutionary history.

The Chandra X-Ray Observatory can easily spot the x-rays coming from regions around black holes in our galaxy and in others, too. Its data has revealed a large number of these cosmic zombies in the Andromeda Galaxy, our nearest spiral neighbor in space. Chandra has spied out 35 black hole candidates seemingly swarming around the center of the galaxy. Seven of those candidates lie dangerously near the core, about a thousand light-years away. Eight black hole candidates are associated with globular clusters, which is an interesting result. The Milky Way’s globulars have not, so far, shown us that they have any black holes.

Now, the interesting thing about Andromeda’s black holes is that in a few billion years, they’ll belong to the Milky Way.  Or, to be more accurate, they’ll be part of a new galaxy that forms when the Milky Way and Andromeda merge. That process will begin in perhaps five billion years and take around 10 billion years to complete. At the end, there’ll be a massive elliptical galaxy containing the stars, black holes, and planets that used to exist in the two separate galaxies.

Want to read more about Andromeda’s newly found black holes? Check out the Chandra X-Ray Observatory Web page for details!

The End of Sun-like Stars

Planetary Nebulae

Several times a year I go out and give public talks about astronomy and one of the questions I get a lot is, “What will happen to the Sun?”  Sometimes people have this idea that the Sun will blow up in a huge explosion and overtake Earth. Others worry about something hitting the Sun and causing it to do something.  Actually, things DO hit the Sun— comets do this, for example. But so far, none has made a difference in how the Sun behaves.

This intriguing new picture from ESO’s Very Large Telescope shows the glowing green planetary nebula IC 1295 surrounding a dim and dying star located about 3300 light-years away in the constellation of Scutum (The Shield). This is the most detailed picture of this object ever taken.
This intriguing new picture from ESO’s Very Large Telescope shows the glowing green planetary nebula IC 1295 surrounding a dim and dying star located about 3300 light-years away in the constellation of Scutum (The Shield). This is the most detailed picture of this object ever taken.

What DOES make a difference in how the Sun (and other stars) acts are age and mass. Stars with masses ranging from one solar mass to about 8 solar masses have fairly quiet deaths — that is, they don’t blow up in titanic explosions so much as they just “puff out” their outer atmospheres to space and then fade away.

The Sun is the one we care the most about. It is about 4.6 billion years old and it will likely live another four billion years before it starts to age and die. That aging process is of great interest to astronomers and so they study other stars as they die to see how the Sun will do it. The Sun and stars like it (similar in mass and luminosity) shine for billions of years before they hit retirement age and start to swell up.

As they do this, their atmospheres get “huffed off” by a stellar wind similar to our solar wind. It’s almost as if the star is gently sneezing its outer layers to space. This takes a while — and all that material eventually ends up in a cloud of gas and dust that surrounds the cloud. That cloud (with the dying star at the center) is what’s called a “planetary nebula”. The name was bestowed by William Herschel, who thought they looked similar to a distant gas giant planet.  There’s nothing planetary about these things — they’re really stars like the Sun moving through an important step in the aging and death process. 

Planetary nebulae come in many different shapes.  This image comes from the European Southern Observatory’s Very Large Telescope. It’s of a nebula called IC 1295, and since the image is such high resolution, you can actually make out multiple shells of material surrounding the dying star. This implies the atmosphere blew out in episodes as the star’s faltering core emitted sudden bursts of energy.

The gas surrounding the dying star (which is the small blue-white spot in the heart of the nebula next to a reddish spot) is bathed in strong ultraviolet radiation from the aging star, which makes the gas glow. Different chemical elements glow with different colors, and the green color you see here comes from ionized oxygen (that is, oxygen gas heated by radiation from the central star and is now emitting greenish light).

This cloud won’t last forever. In a few tens of thousands of years, the clouds will slowly dissipate. Eventually only the remains of the star will be left behind as a white dwarf.  It will continue to shrink a bit longer, but eventually that will stop and the white dwarf will continue to cool for billions of years. I read somewhere that in the entire history of the universe, not one white dwarf has yet cooled to completion. There hasn’t been time in the 13.8-billion-year age of the cosmos for them do that.

So, that’s the fate of the Sun in general. It won’t blow up as a supernova (because it doesn’t have the mass to do so). It will gently (for a star) sigh its life away. Hopefully by that time, humanity will have found other worlds to live on.