The Cat’s Eye Nebula – Credit: NASA, ESA, HEIC, and The Hubble Heritage Team (STScI/AURA)
(Click the image for a larger version)
Hubblesite.org: The Cat’s Eye Nebula, one of the first planetary nebulae discovered, also has one of the most complex forms known to this kind of nebula. Eleven rings, or shells, of gas make up the Cat’s Eye.
We recently checked out Supernova 1987A. If you remember, I told you that when massive (8 times the mass of the Sun or greater) stars die they explode in a supernova and leave behind either a neutron star or a black hole, surrounded by a supernova remnant.
When a low mass star (less than 8 times the Sun’s mass) dies, it leaves behind a white dwarf and a planetary nebula. An example of which is shown above, the Cat’s Eye Nebula (also designated NGC 6543). 4 or 5 billion years from now, our own Sun will undergo this very same process.
Perhaps our distant ancestors, or even members of an alien species, will look towards the vicinity of our former home in the galaxy and capture an image just as beautiful.
When we think of what it takes to be a scientist, we imagine many torturous years or studying, research, and education. While that certainly might be the path for a Ph.D. in a field of science, it certainly isn’t required to do science. In all actuality, we do science everyday; most of the time without even thinking about it.
For now, I want you to think about doing some science; science that will help many other scientists around the globe. It’s quick, easy, and fun. Participate in the 2012 Globe At Night.
Globe At Night relies on scientists around the globe, including amateurs, to make simple observations of the night sky in their area. The purpose is to obtain useful data on light pollution and astronomical viewing. Light pollution has a number of detrimental aspects, from negative affects on wildlife to issues regarding energy consumption. Most apparent to skygazers such as myself and many of you, light pollution is quickly degrading our view of the starry night sky. Globe At Night’s mission is to raise awareness about light pollution and collect data to measure its current impacts.
So contribute your scientific skills to the effort! All you really have to do is go outside, look at the constellation Orion (which is one of my favorites and worth viewing just for the sake of viewing it), and then compare your view with the charts provided. Globe At Night has a very user-friendly interface for recording the data, and they even offer smartphone applications (check your market for “Globe At Night”). After that, check out the map that integrates all of the data already being collected around the planet and find out where on Earth you’ll see the darkest skies.
There are four opportunities to participate this year, and the first is currently happening now (January 14 to 23). So please do it now! The next opportunities will be: February 12-21, March 13,22, and April 11-20.
Today, the Earth will be at a point in its orbit around the Sun called perihelion; the point in its orbit about which it is closest to the Sun. Until early July, we’ll be getting further and further away from the Sun, after which point we start getting closer again.
The overall change in distance is quite small, comparatively. Today, we’re approximately 3.1 million miles (just shy of 5 million kilometers) closer to the Sun than we will be in July, at aphelion. When you compare that to an average distance of around 93 miles, you’ll realize why the change in distance is virtually unnoticed by us Earthlings (unless we’re scientists specifically studying the Sun).
With so many wondrous space-related images being captured on a daily basis, it is difficult to single any out as “the best”. That said, there are those that just stick in your mind… the images that run through your head when you’re trying to go to sleep, that make you ask questions, that inspire you to spend hours doing research, and those that make your jaw drop to the floor. Here are a small handful of the ones that have done that to me this year.
I hope you enjoyed these as I have, and I look forward to what 2012 has in store for us!
Astronomy Picture Of The Day: Explanation: The yellowish star near center in this remarkable telescopic skyview is T Tauri, prototype of the class of T Tauri variable stars. Nearby it is a dusty yellow cosmic cloud historically known as Hind’s Variable Nebula (NGC 1555). Over 400 light-years away, at the edge of a molecular cloud, both star and nebula are seen to vary significantly in brightness but not necessarily at the same time, adding to the mystery of the intriguing region. T Tauri stars are now generally recognized as young (less than a few million years old), sun-like stars still in the early stages of formation. To further complicate the picture, infrared observations indicate that T Tauri itself is part of a multiple system and suggest that the associated Hind’s Nebula may also contain a very young stellar object. The naturally colored image spans about 4 light-years at the estimated distance of T Tauri.
Saturn has moons. Lots of moons (at least 62). And I find each one of those moons to be equally interesting.
Recently, the orbiter, Cassini, snapped the following photo of one of Saturn’s moons, Mimas.
(Click image to BIGGIFY)
Mimas is the twentieth largest moon in our solar system, yet is the smallest astronomical body that is believed to be round in shape due to its self-gravitation. Mimas has an interesting feature in a huge crater named Herschel. Compared to Mimas, this crater is huge. It is 80 miles (130km) wide, which is about a third of the total size of the moon itself (wider than Canada). As Phil Plait points out, the impact that created this crater was just about as big as it could have been without obliterating Mimas.
The results are beautiful. Some see the crater resembling a big eye. To many, including myself, it looks like the Deathstar:
(That’s no moon. It’s a space station. – Obi-Wan Kenobi)
For a mission that began in 1997, Cassini (Cassini-Huygens originally, until the Huygens probe was sent to land on the surface of Titan) just keeps on keepin’ on. It has had its missions and extended multiple times, and will most likely keep snapping these shots until it makes a flaming plunge into Saturn’s atmosphere in 2017. NASA, and its counterparts from around the globe, have done a fantastic job of completing their main missions, and then coming up with ways to continue using them for additional missions. We’re learning new and amazing things on a regular basis, and I think that’s just grand.
The following video is my first real attempt at time-lapse astrophotography. I chose one of my favorite constellations, Ursa Major (best known for containing The Big Dipper). The video shows the motion of the constellation over a 45-minute period.
I live in a small city, so some light pollution factored into the result but overall the night was quite clear. You can clearly make out “The Horse and Rider”, two stars that make up what is typically seen as the second star in The Big Dipper’s handle. The ability to see these two stars, Mizar and Alcor, was used by the Arabs, Romans, and English to test the eye-sight of their warriors.
But there’s even more to Mizar and Alcor than meets the (unaided) eye. Mizar is actually a quadruple system of two binary stars and Alcor is a binary system. Together, they make up sextuple system, as they are all apparently gravitationally bound.
To put it simply, Mizar — which we see as the brighter star, the horse, making up the Horse and Rider — is two sets of two stars orbiting each other. Alcor, is a single set of two stars orbiting each other, and is in turn interacting with the Mizar system. Six stars, dancing together in a cosmic folk dance, appearing to us on Earth as one or two stars (depending on your eyesight).
Additionally, this all goes to show that as much as we think we know about the cosmos, there is so much more out there to discover. Mizar and Alcor have been two of the most observed objects in the night sky for millennia, yet we still continue to unravel more of their magic.
The Black Eye Galaxy (Messier 64), in the constellation Coma Berenices, is a spiral galaxy, visible with even a small telescope. It was discovered in 1779, by Edward Pigott (and independently a month later by Johann Elert Bode and in 1880 by Charles Messier). In a majority of galaxies, the stars all orbit in the same direction. Interestingly though, the gases in the outer region of M64 rotate in the opposite direction of the gases and stars within the inner region. To clarify the scale, the inner region has a radius of 3,000 light years, while the outer region extends an additional 40,000 light years. (That’s big, but take note that M64 is 19,000,000 light years from Earth.) The boundary between the two regions is believed to trigger a very productive birthing ground for many new stars. Astronomers believe that this pattern was caused when M64 absorbed a satellite galaxy brought in on a collision course, approximately 1 billion years, or more, ago.
The darkened band that gives the galaxy it’s nickname is a dust feature that’s obscuring the light from the nucleus of the galaxy.
The red giant AFGL 3068 is dying a beautiful death. Like all red giants, as they expand they spew their outer layers into space in a spherical shape. What’s unique about AFGL3068 however, is that it’s actually a binary star — two stars orbiting each other. Due to the orbits of the two stars, the material that’s ejected isn’t able to expand into a sphere, but in this amazingly perfect (and awesomely huge at 3 trillion kilometers!) spiral.
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