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This week we continue the story of galaxy formation, learning how groups of galaxies come together to form the biggest structures around - galaxy superclusters. And when you look at the Universe at this scale, environment is everything.
Read the full blog entry |
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If you want to download the mp3 or the 16kb version of any show, you can always visit our archive for a listing of all our shows and links to download in the format of your choice. Additionally, there are links at the top of each episode's page to allow you to download the mp3 if you'd prefer it to then m4a. The mp3 will always be a much smaller file. Hope that helps. -Rebecca Astronomy Cast Student Worker |
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Hum,
tnx, i didn't realise there was an economy class Internet connection link available (14mb, mp3).
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`Irony` actually does mean `metal like`... |
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We've thought of everything. :-)
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Fraser Cain Publisher Universe Today - Free space news delivered by email every weekday. |
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Hey guys,
Just listened to the show - it was as good as ever. Thanks! This weeks show reminded me of a recent APOD showing the galaxy cluster showing Abell 2667. Its got a great example of galaxy 'harassment' (haha - a new one for me!) and some lovely lensing. What a picture. How we're gonna miss hubble! http://antwrp.gsfc.nasa.gov/apod/ap070305.html Might be worth adding to show notes? Anyway, thanks again. Looking forward to next weeks show. Andrew (Belfast, Northern Ireland) |
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I just added a "pretty pictures" category to this week's show notes. I try to include a bunch of cool pictures in the HTML version of the transcript (below the show notes) but now I've linked to some of the sites that I get those pictures from so you can browse to your heart's delight! -Rebecca Astronomy Cast student worker |
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ok I have listened to the first 32 podcasts and this episode is the one that I have a question about. I am asking this from a point of knowing I do not understand a lot, but here goes...
Why do super large galaxies have an elliptical shape and smaller ones are disc shaped? Here is why I ask, the milky way, for example is spiraling around a super massive black hole, so is the Andromeda Galaxy. Systems within the Galaxies have stars rotating around stars, planets rotating around stars, black holes consuming gas in a spiraling accretion disk etc. The effects of angular momentum is readily apparent on scales as small as a planet/moon relationship, all the way up to our galaxy. So why is it, that large galaxies lose this trait? For that matter, why are galaxies clustered in a sponge-like pattern instead of in an ever larger spiral? Is there an upper bound on the effects of angular momentum and ultra-large collections of mass or has there just not been enough time for these effects to take place? Or maybe they HAVE taken place but it hasn't reached us yet? Also, in a similar vein, why are globular clusters not disk-shaped? what is it about their structure that keeps them from spinning up around a denser core group? Awesome podcasts, by the way. I love this series, and have to say that Fraser and Pam discuss things on a level that isn't too high fr a layman such as myself to understand. |