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Old 07-October-2006, 07:52 AM
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Default Supernova radioisotopes show solar system formed next to a supernova

From Spaceref, this is an interesting press release, evidence is presented that the solar system formed in very close proximity to a massive star that exploded as a supernova, which would mean the sun was born in a dense star cluster, as massive stars are unlikely to form elsewhere and don't wander too far before exploding. The speculation has been building to this conclusion for a while now.
Quote:
PRESS RELEASE
Date Released: Thursday, October 5, 2006
Source: University of Illinois at Urbana-Champaign

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CHAMPAIGN, Ill. -- The death of a massive nearby star billions of years ago offers evidence the sun was born in a star cluster, say astronomers at the University of Illinois at Urbana-Champaign. Rather than being an only child, the sun could have hundreds or thousands of celestial siblings, now dispersed across the heavens.
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Old 07-October-2006, 12:42 PM
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This isn't an especially new idea, but I'm glad that they are continuing to look for details in this history. It will be interesting to look for the siblings. Other stars roughly co-moving with us in our orbit of the Milky Way, all with ages between say 4.8 and 4.4 billion years. I give this spread in age not really knowing the duration of a star-forming region either now, or 5 billion years ago during the long height of star formation in the Milky Way.
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Old 07-October-2006, 12:54 PM
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Question massive stars

This is interesting. I've seen a number of articles suggesting that massive stars(supernovae progenitors) are far more frequently formed from large dust & gas regions of relatively low density...such as the periphery of the galactic arms, and halo....and that dense regions cause multiple smaller stars to form, red dwarfs, G, K's... Evidently the thinking has changed here? If so, the greatest majority of supernova remnants should be found towards, and in the galactic bulge. I'm not sure that's correct. Hmmm. Pete.
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Old 08-October-2006, 05:40 AM
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This is even on our website's front page, and I had to hear about it here. That's a cool thing, though. I wish John would have told me what he was working on.
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Old 08-October-2006, 11:36 AM
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Hum,

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Old 08-October-2006, 11:50 AM
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Quote:
Comparisons between the predicted abundances of short-lived radioactive nuclides (107Pd, 129I, 182Hf, and 244Pu) in the interstellar medium (ISM) and the observed abundances in the early solar system have conclusively showed that these nuclides cannot simply be derived from galactic chemical evolution (GCE), if synthesized in a unique stellar environment.
It was thus suggested that two different types of stars were responsible for the production of light and heavy r-nuclides.
However, new constraints on the 244Pu = 238U production ratio used in an open nonlinear GCE model, show that the two r-process scenario cannot explain the low abundance of 244Pu in the early solar system, and that this requires either than actinides be produced at an additional site, or more likely, that 129I & 244Pu be inherited from GCE and 107Pd & 182Hf be injected in the early solar system by the explosion of a nearby supernova.
http://xxx.lanl.gov/PS_cache/astro-...502/0502514.pdf
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