Happy Valentine's Day From the Folks at Spitzer Space Telescope
Wanna surprise your sweetie with a cosmic valentine? You can’t go wrong with this lovely image of the Ring Nebula (Messier 57), as seen by the Spitzer Space Telescope. It makes a lovely picture to show off, right after you present your loved one with whatever special surprise you have planned for the holiday.
Spitzer Space Telescope is an infrared facility, meaning that it sees wavelengths of light just beyond those we can see with our eyes. The objects that give off infrared light are often dusty and warm, which explains the way the Ring Nebula looks. It’s a planetary nebula, a shell of material ejected from a dying star. The ring is actually a thick cylinder of gas and dust blown off by the dying star early in its death agonies. Radiation from the star heats up the shell of gas, causing it to glow—and that’s what makes the Ring Nebula look so beautiful and ghostly in the infrared.
If you want to look at this ring in greater detail, check here for links to larger, higher-resolution images. It’s an amazing site to behold, and definitely something different to share with your sweetie.
Back when I used to lecture in the planetarium I would solicit questions from the audience at the end of each presentation. Every once in a while somebody would ask me what it’s like inside a black hole.
Trick question, right?
Well, probably for some of the more smart-aleck audience members it was. But, I always had an answer. I’d go into a little discussion about how we don’t know exactly, and based on a number of factors (including the laws of physics, some Einsteinian laws, etc.), we’ll probably never have a chance to explore the inside of one (and, if the gravity is so strong that light can’t even escape, is the inside of a black hole REALLY a place we want to be?). Following that there’d be a silence as people digested the idea of “being there”. Then we’d get into a discussion about what it be like to be right next to a black hole, which is a lot easier to describe, even if it IS a shrieking maestrom of radiation and searing temperatures.
At the time I was first in school, back in the dark ages of the early 60s, black holes were sort of a mathematical curiosity, a physics problem for which we didn’t have any good examples. That all changed with the advent of telescopes and detectors able to “see” the effects of black holes, including the jets that spray out from the vicinity of one as matter (stars, gas, dust) spiral into the hole. Moreover, black holes have gravitational effects on nearby stars and gas and dust that we CAN track with spectroscopic observations of the light emanating from the nearby region.
The Milky Way's Black Hole Courtesy European Space Agency's Integral Mission
Which brings us to the center of our own galaxy, where a supermassive black hole about a million times the mass of our Sun lies hidden by gas and dust clouds and star clusters. This SMBH (for short), also known as Sagittarius A* (or SgrA*), radiates tremendous amounts of energy which we can detect in gamma rays. As luck would have it, we have a spacecraft called INTEGRAL that “sees” that radiation. In the image above, INTEGRAL shows us a gamma-ray view of the region near the center of the Milky Way.
Now, SgrA* is a pretty quiet and harmless black hole, and isn’t quite the powerhouse of radiation that others are—like, say, the black hole at the center of galaxy M87, which sports a very active jet. Yet, in the past, the Milky Way’s resident black hole has been restless, and whenever it acts up, the surrounding clouds light up with the evidence.
Right near SgrA* is a cloud of gas called SgrB2, and the two are about approximately 350 light-years apart. Sgr B2 is being exposed to a blast of gamma rays emitted by Sgr A* that went off about 350 years ago. The cloud absorbed the radiation and has been emitting it. Interestingly enough, the astronomers studying the data think that the whole outburst took at least ten years, possibly longer. And they’re using their studies to figure out how often and how strongly “our” black hole turns on, radiates, and then turns off again.
I have to admit, it’s pretty heady growing up knowing that these weird things that scientists once thought were probably rare are now found all over the place (in many galaxies and at the death scenes of supermassive stars). And, I find it very cool indeed that we can study the near-black-hole environment and learn so much about them.
