Thursday, September 3, 2015

Newscenter Update: Hubble Survey Unlocks Clues to Star Birth in Neighboring Galaxy

September 3, 2015
Star Clusters in the Andromeda Galaxy
Get larger image formats
 

Find the entire Hubble News archive, image galleries, and much more at hubblesite.org

Stay Connected
 
Hubble Survey Unlocks Clues to Star Birth in Neighboring Galaxy

All stars are not created equal. They can vary in mass by over a factor of 1,000. Our sun is classified as a diminutive yellow dwarf. What's more, stars are not born in isolation, but inside giant molecular clouds of hydrogen. The question has been: what fraction of stars precipitate out of these clouds into clusters that contain blue giants, yellow dwarfs, and red dwarfs? It's like asking if all automobile manufacturers fabricate the same proportion of trucks, SUVs, sedans, and subcompacts. The best way to address the question is not to look around our Milky Way — which we are inside — but far out into space to the neighboring Andromeda galaxy, 2.5 million light-years away. Embedded in a sweeping Hubble Space Telescope mosaic of 117 million stars in the galaxy's disk are 2,753 star clusters. Hubble astronomers found that, for whatever reason, nature apparently cooks up stars like batches of cookies. There is a consistent distribution from massive stars to small stars. It is surprising to find that this ratio is the same across our neighboring galaxy (as well as inside our stellar neighborhood in the Milky Way), given the complex physics of star formation.

RELEASE LINKS: arrowSee full release
arrowMore Images
arrowFast Facts

This news release and its supporting materials are permanently achived at: http://hubblesite.org/newscenter/archive/releases/2015/18/

You are receiving this email because you are subscribed to the Inbox Astronomy mailing list, which sends notices in HTML whenever there is a new Hubble Space Telescope image, product, or news update. If you would like to unsubscribe or change your email preferences, please go to: http://hubblesite.org/newscenter/hubble_on_the_go/inbox_astronomy/

No comments: