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I read somewhere that the sun is part of an open cluster. If thats true,
wouldn;t it have to be awefully OLD for an open cluster? What other stars are in the cluster? How many? How large is it? Any nebula still left? thanks jjb |
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Jeremiah J. Burton wrote:
I read somewhere that the sun is part of an open cluster. If thats true, wouldn;t it have to be awefully OLD for an open cluster? What other stars are in the cluster? How many? How large is it? Any nebula still left? More precisely, the Sun was almost certainly formed as part of such a cluster (based on virtually all young stars we see today coming in clusters and associations). Open clusters lose their identities over time, for at least two reasons. First, the more of the remaining gas is blown away by the most massive cluster members (including their supernovae), the less mass is left to hold the whole cluster together gravitationally. On top of that, random encounters with stars and massive interstellar clouds will strip stars away over time. These are reasons that there are very few open clusters known to nearly as old as the Sun (M67 and NGC 188?), and the number increases rapidly for smaller ages. By now, Sol has lost track of the siblings, although there are a few nearby stars with similar enough space motions that they might share a common origin. Bill Keel |
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Fellow Iowan Sam Wormley was saying
Several of the stars in the "big dipper" have similar motions about the galaxy as our sun. Seems like I can remember reading long ago that Sirius seemed to be moving along with this group too. Marty |
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Marty wrote:
Fellow Iowan Sam Wormley was saying Several of the stars in the "big dipper" have similar motions about the galaxy as our sun. Seems like I can remember reading long ago that Sirius seemed to be moving along with this group too. Marty I believe I've read that too. There is some doubt that any of the stars mentioned in the this thread are the remnants of the original cluster... mostly because the spectral types imply big age differences. |
#5
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![]() "Jeremiah J. Burton" wrote in message s.com... I read somewhere that the sun is part of an open cluster. If thats true, wouldn;t it have to be awefully OLD for an open cluster? What other stars are in the cluster? How many? How large is it? Any nebula still left? I am amazed no one has mentioned Alpha C - A B and C for starters. At 4.36- 4.5 LYs away, they sure do qualify. Alpha C A is some 7 Billion years old that again qualifies. The sun is 5-6 Byrs. http://www.alphacentauri.org/centauri.html |
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On Fri, 21 May 2004 01:42:24 GMT, "Thomas" wrote:
I am amazed no one has mentioned Alpha C - A B and C for starters. At 4.36- 4.5 LYs away, they sure do qualify. Alpha C A is some 7 Billion years old that again qualifies. The sun is 5-6 Byrs. Based only on the system's nearness? It has a very high proper motion which might argue against formation in the same cluster as the Sun (hint: plot the proper motion backwards 5 billion years; is the system still close?) Also, if the stars are a billion years or more older than the Sun, that argues against a common origin, since star forming regions typically have lifetimes measured in millions of years, not billions. _________________________________________________ Chris L Peterson Cloudbait Observatory http://www.cloudbait.com |
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Chris L Peterson wrote:
Based only on the system's nearness? It has a very high proper motion which might argue against formation in the same cluster as the Sun (hint: plot the proper motion backwards 5 billion years; is the system still close?) Anyone have a list of nearby stars with U/V/W velocities? Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
#9
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Brian Tung wrote:
Anyone have a list of nearby stars with U/V/W velocities? You may already know this, but the Yale Bright Star Catalog lists both proper motion and radial velocity, along with position (of course) and parallax. It should be straightforward to get a cartesian vector from that. The initial position in spherical coordinates is P0 = (ra, dec, s) where s, the distance in parsecs, is 1 / parallax. The position after time t is P1 = (ra + pra, dec + pdec, s + v) where (pra, pdec) is the displacement due to proper motion and v is the displacement due to radial velocity. Convert P0 and P1 to rectangular coordinates and subtract to get the velocity vector (the displacement in rectangular coordinates over time t). - Ernie http://mywebpages.comcast.net/erniew |
#10
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Ernie Wright wrote:
You may already know this, but the Yale Bright Star Catalog lists both proper motion and radial velocity, along with position (of course) and parallax. It should be straightforward to get a cartesian vector from that. Yes, but I was hoping not to have to do all that pesky work. Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
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