Astrowiki/Spiral Galaxies
From BluWiki
|
This Page is Part of Astrowiki
Contributions wanted. - BluWiki is unique in that original page authors normally decide who can edit their page. By putting this banner up, the author(s) of this page are soliciting your assistance. Please help them by contributing useful information to it. You might find more information about what is wanted in the discussion of this page.
|
Contents |
Intro
A spiral Galaxy is a type of galaxy distinguished by it's shape of multiple spiral arms coming inwards into a central bulge.The bulges almost always contain a supermassive black hole that is billions of solar masses in size. Some of the largest galaxies that we know of are spirals . Our galaxy is a spiral along with larger Andromeda Galaxy.In the outer boundary of a spiral Galaxy there is a halo of older stars.
Bulge
The bulge contains old , population 2 stars and resembles an elliptical galaxy. Many of the stars in the bulge are red giants . Occasionally a "starburst" event ,a flood of incoming matter causing a burst of star formation , will occur.
Spiral Arms
The arms rotate around the bulge and are made up of young population 1 stars . Open Star Clusters are common in the disc and are made up of up to 10000 stars. We live in the Arms of a spiral Galaxy
Halo
The halo of matter at the edge of a spiral Galaxy is made up of old population 2 stars in massive globular clusters that contain up to 10000000 stars
References
"Spiral Galaxy." Wikipedia. 16 Aug. 2007 <http://en.wikipedia.org/wiki/Spiral_galaxy>.







