Great Balls of Low Entropy Gas Fire!

By Aaron on July 31, 2006 at 12:16 pm | In Slacker Astronomy Archival Podcasts | No Comments

Why? Well why not? If you were a bored bit of gas living out your days in the suburbs of such a great galactic metropolis, wouldn’t you too want to take a plunge, and go live in the center of things for a while?

Show Notes:

SA Extra: Chit Chat #10

By Aaron on July 25, 2006 at 8:12 pm | In Slacker Astronomy Archival Podcasts | No Comments

from Doug: “Regarding the M81 question, it would be worth mentioning that none of
foreground stars that adorn all in-Milky Way based images of external
galaxies would be visible to the observer sitting in intergalactic space!”

The blazar: 2 oz vodka, 4 oz OJ, 1 oz grenadine…

Ring around the Planet (Show #59)

By Slacker on July 20, 2006 at 10:20 am | In Slacker Astronomy Archival Podcasts | No Comments

Show Notes

And now for some pictures…
Saturn’s double banded E-Ring (credit: NASA/JPL/Space Science Institute)

Persistent Arc at the edge of Saturn’s G-ring. (credit: NASA/JPL/Space Science Institute)

And in finally ….

Dancing Moons

Finders Keepers (Show #58)

By Aaron on July 11, 2006 at 7:44 pm | In Slacker Astronomy Archival Podcasts | No Comments

Castdate: 060711
Title: Finder’s Keeper’s
Written By: Aaron
Disembodied Voices: Pamela, Travis, Rebecca
Engineered By: Travis
Rating: [OF] Office Friendly

And then there was dust … (Show #57)

By Slacker on July 6, 2006 at 6:47 pm | In Slacker Astronomy Archival Podcasts | 8 Comments

Images Credit: NASA/JPL-Caltech/B.E.K. Sugerman (STScI)

Show notes:


From the Spitzer website: “The dust factory, also known as supernova SN 2003gd, is shown at the center of the two small insets from Spitzer’s Infrared Array Camera (IRAC). A white arrow points to its exact location. The yellow-green dot shown in the July 2004 inset (top) shows that the source’s temperature is warmer than the surrounding material. This is because newly formed dust within the supernova is just starting to cool. By January 2005, the dust had cooled and completely faded from IRAC’s view. However, it was still detected in January 2005 by another instrument aboard Spitzer called the Multiband Imaging Photometer (MIPS). The MIPS image is not shown here.

The larger image to the right of the insets is the galaxy M74, as seen by Spitzer’s Infrared Array Camera. The white box to the left of the galaxy’s center identifies the location of the supernova remnant. In all the images, the blue dots represent hot gas and stars. The galaxy’s cool dust is shown in red.

The images are false-color, infrared composites, in which 3.6-micron light is blue, 4.5-micron light is green, and 8-micron light is red.

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