TheSpacewriter

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These pages chronicle the work and ruminations of Carolyn Collins Petersen, also known as TheSpacewriter.

I am vice-president of Loch Ness Productions. I am also a producer for Astrocast.TV, an online magazine about astronomy and space science.

For the past few years, I've also been a voice actor, appearing in a variety of productions. You can see and hear samples of my work by clicking on the "Voice-Overs, Videos and 'Casts tab.

My blog, TheSpacewriter's Ramblings, is about astronomy, space science, and other sciences.

Ideas and opinions expressed here do not represent those of my employer or of any other organization to which I am affiliated. They're mine.

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**Comments are welcome; I do moderate them to weed out spam.

Contact me for writing and voice-over projects at: cc(dot)petersen(at)gmail(dot)com

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Blog entry posting times are U.S. Mountain Time (GMT-6:00) All postings Copyright 2003-2010 C.C. Petersen


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« Galaxy-building Exercises
Friday Musings »


The Cosmic Dance

Galactic Minuets

Yesterday I talked about galaxy mergers and acquisitions, the subject of my latest segment on Astrocast.tv. These scenes fascinate me because galaxies are not exactly tiptoing through the tulips as they interact with each other.

Think of the sheer amount of mass involved!  For the Milky Way, you’re talking about the mass of what, somewhere between 300-400 billion stars.  If every star in the galaxy had the same mass as the Sun — which has a mass of 1.9 x 1030 kilograms — you’re talking about a LOT of mass. Of course, not every star is the mass of the Sun — some are more massive, some are less massive. And, of course, we have that pesky massive black hole at the center, and huge amounts of interstellar gas and dust also poking around the space lanes.

When two galaxies interact, however, that mass doesn’t all clash together in a huge crash.  Stars aren’t necessarily colliding with each other, although the action of the merger does compress the interstellar gas and dust, and sets off waves of star formation. But, all of that mass exerts a gravitational influence, which is the main “actor” in a galaxy collision.  That influence is what tears out streams of gas and dust from interacting galaxies, and reshapes the morphology (the shape) of all the galaxies doing the interacting.  While a galaxy interaction may look graceful in the images we see from HST and Spitzer and other observatories, it’s quite a massive and impressive undertaking.

To understand how these collisions and interactions take place, astronomers are creating impressive computer models. These get turned into animations that allow us to follow the galactic dance from start to finish, many many times faster than it happens in real life.  I used one from a scientist named John Dubinksi in my segment (see it below) to show the upcoming Milky Way/Andromeda Galaxy interaction, which will happen in our far future. Check it out!  And, head over to Astrocast.tv to see the rest of this month’s space news show!

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This entry was posted on Tuesday, June 2nd, 2009 at 12:16 pm and is filed under astrocast.tv, galaxies, galaxy interactions. You can follow any responses to this entry through the RSS 2.0 feed. You can leave a response, or trackback from your own site.

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  1. Galaxies tiptoeing though tulips… that’s an adorable mental image!

    Comment by Nicole — June 7, 2009 #

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