Difference between revisions of "Milky Way"
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| − | The [[Milky Way]], home to the [[Solar System]], is one of the densest, most massive spiral galaxies known, and the dominant member of the [[Local Group]] by mass. While its stellar disc is physically smaller than [[Andromeda]]'s, our home galaxy has about half again the mass of its already giant neighbor, at least [http://adsabs.harvard.edu/cgi-bin/bib_query?2000MNRAS.316..929E 1.9 trillion Solar Masses], about a third of which is baryonic, and half of that luminous. This suggests a total stellar population around 600 billion, but could be as high as a few trillion. | + | The [[Milky Way]], home to the [[Solar System]], is one of the densest, most massive spiral galaxies known, and the dominant member of the [[Local Group]] by [[mass]]. While its stellar disc is physically smaller than [[Andromeda]]'s, our home [[galaxy]] has about half again the mass of its already giant neighbor, at least [http://adsabs.harvard.edu/cgi-bin/bib_query?2000MNRAS.316..929E 1.9 trillion Solar Masses], about a third of which is baryonic, and half of that luminous. This suggests a total stellar population around 600 billion, but could be as high as a few trillion. |
An extremely pronounced bar structure appears to dominate the central region of the [[Milky Way]], suggesting that the [[galaxy]] has yet to encounter a major collision event, though eventually [[Andromeda]] will make such a collision. | An extremely pronounced bar structure appears to dominate the central region of the [[Milky Way]], suggesting that the [[galaxy]] has yet to encounter a major collision event, though eventually [[Andromeda]] will make such a collision. | ||
Revision as of 09:55, 1 May 2006
The Milky Way, home to the Solar System, is one of the densest, most massive spiral galaxies known, and the dominant member of the Local Group by mass. While its stellar disc is physically smaller than Andromeda's, our home galaxy has about half again the mass of its already giant neighbor, at least 1.9 trillion Solar Masses, about a third of which is baryonic, and half of that luminous. This suggests a total stellar population around 600 billion, but could be as high as a few trillion.
An extremely pronounced bar structure appears to dominate the central region of the Milky Way, suggesting that the galaxy has yet to encounter a major collision event, though eventually Andromeda will make such a collision.
