Universe Today - September 6, 2005

The New Forum is Online
Sep 6, 2005 - As I mentioned a few days ago, Phil Plait from Bad Astronomy and I have decided to merge our two forums into one super-space forum. The new forum is now live, and accessible from http://www.bautforum.com. This new forum has more than 10,000 members, and almost 550,000 posts.

Although the forum is functional and ready for conversations, we'll still be tweaking it over the next few days, weeks, months. Let us know if you find any bugs. Please also let us know if you're having any problems logging in with your username.

I look forward to seeing you there.

Fraser Cain
Publisher
Universe Today (Full Story)
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NGC 6822. Image credit: Local Group Galaxies Team/NOAO/AURA/NSF. Click to enlarge.
What's Up This Week - September 5 - September 11, 2005
Sep 6, 2005 - Greetings, fellow Sky Watchers! While the Moon will figure prominently in our studies this week, let's start off with telescopic challenge - "Barnard's Galaxy". Do you only have binoculars? Don't worry, the NGC 6871 will surely please you. If you have eyes, then you're in luck as the Moon, Jupiter, Venus and Spica dazzle the western skyline and Piscid meteor comes to call. So, get thee out under the stars and in the moonlight, because...

Here's what's up! (Full Story)
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Image credit: Mike Salway. Click to enlarge
Astrophoto: Crux and Centaurus by Mike Salway
Sep 6, 2005 - Mike Salway took this picture of Crux and Centaurus on the 9th July, 2005 from Kulnura, on the Central Coast of NSW, Australia. This image was taken with a Sony Cybershot 5.1mp digicamthe and is a result of 5 images @30s each (ISO400).

Do you have photos you'd like to share? Post them to the Universe Today astrophotography forum or email them to me directly, and I might feature one in Universe Today.
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Saturn Rings. Image credit: NASA/JPL/SSI Click to enlarge
Cassini Scientists Make New Ring Discoveries
Sep 6, 2005 - Cassini scientists have announced a host of new findings about Saturn's rings, including some new knotted structures in the planet's F ring. One of the major discoveries is that parts of Saturn's D ring (its innermost ring) have relocated and dimmed. In fact scientists have been able to track fairly significant changes between when Voyager first visited Saturn 25 years ago. The delicate G ring seems to contain faint arcs, which might be hiding additional planets. And most surprisingly, knots in the planet's F ring seem to be arranged like a coiled spring winding around the planet. (Full Story)
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Artist's impression of a pulsar 'eating' a companion star. Image credit: ESA Click to enlarge
Star Gobbles Up Its Friend
Sep 6, 2005 - The ESA's Integral space observatory and NASA's Rossi X-ray Timing Explorer spacecraft have found a rapidly spinning pulsar in the process of consuming a neighbour. This discovery supports the theory that pulsars spin so quickly because they pick up material from a companion, which increases their mass. Pulsars were once stars more than 8 times as large as our Sun, but their intense gravity compacted them down to a size of about 20 km (12 miles) across. (Full Story)
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Moon Pandora from outside Saturn's F ring. Image credit: NASA/JPL/SSI Click to enlarge
Pandora Shepherding the Rings
Sep 5, 2005 - In this photograph taken by Cassini, you can see the faint moon Pandora moving through Saturn's F ring. As a shepherd moon, Pandora and its partner Prometheus confine and shape the main F ring with its gravity. Pandora is 84 kilometers (52 miles) across. This image was taken on August 2, 2005, when Cassini was approximately 610,000 kilometers (379,000 miles) from Pandora. (Full Story)
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Supernova Remnant N 63A. Image credit: Hubble Click to enlarge
Building Life from Star-Stuff
Sep 5, 2005 - There's a long chain of events that led from the collapse of our local cloud of gas and dust to the evolution of life here on Earth. Exactly how each of these steps unfolded is still a bit of a mystery, but scientists know that a few atomic combinations were necessary: water, and organic compounds containing carbon. Dying stars are the source for this carbon, which they belch out, creating a kind of carbon soot. From there, this soot is blasted by intense radiation to create more than 100 different molecules, including fatty acids and simple sugars. (Full Story)
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