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Our Sun is considered a third generation star. What happened to generations 1 and 2? Obviously, some catastrophic event (supernova) must have happened and then all the "stuff" coalesced and we did it again. Here's my question, "What's the possibility that an earlier solar system existed, possibly with life, in those two prior generations? And since the universe is 14 BYO and our sun is about 4.6 BYO, that leaves almost 10 BY for two systems to have existed and then died. That's enough time for life to exist, isn't it?
And what elemental composition percentages make us sure that our sun is a 3rd generation star? Is it the composition of the heavy metals, those heavier than iron? Thanks. |
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Quote:
Even 3rd-generation Population I stars and systems are mostly hydrogen and helium, but they contain enough other elements to build more variety. The previous generations of stars lived their lives. Some 2nd-generation Population II stars are still about. The ancient Population III stars are gone. Introductory material can be had at NASA Worldbook :: Star and :: Sun. Also, Wikipedia: Metallicity looks good. And, welcome to the BAUT Forum.
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Him, that's actually a good idea for an episode. We'll cover the various stellar populations.
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Fraser Cain Publisher Universe Today - Free space news delivered by email every weekday. |
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its it a thought that the very first stars were nearly totally made of Hydrogen and bigger than even Eta Corina with lifespans of only 100,000 years or so before they blew apart (litterally leaving nothing - not even blackholes).
10,000,000,000 minus 100,000 yrs leaves a very large number and plenty of time for more metal production. Heard on NPR "stardate" that the above 1st gen. stars and the rare hyper-giants of today like Eta Carina leave no core to collapse - they totally blow apart in full. I had never heard of that before - I had always thought that bigger = black hole after supernova all these years. |
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