@oralloy,
oralloy wrote:
The material didn't arrive. It was here already.
Ok, you said it "arrived long ago," and now you say "it was already here." I am talking about what it was traveling 'long ago,' not after it was 'already here.'
Quote:It likely cooled pretty fast. Space is cold.
I'm trying to get a little more specific in terms of how fast a supernova's material cools as it is expanding outward from the blast center.
Quote:The origins of the supernovae (probably plural) are lost to ancient history. This was a long time ago.
So was the big bang, but people trace back the evolution of the universe in its direction (which is actually all directions, according to the theory).
Quote:Some of the stellar remnants of the supernovae that created our raw material might now be part of the Milky Way's central supermassive black hole. But there is no way to know for sure.
I'm no expert, but I think it would make sense to look at some other supernovae and estimate at what distance material emanating from them cools and falls into orbit around other stars, such as the sun.
I assume that if we were 'fresher supernova ash,' there would be more material closer to us in our region of the galaxy. The further the supernova spreads out, the less dense it gets.
If what you're saying is right, that multiple supernovae contributed material from different directions, then the question becomes what form the 'ashes' took as they traveled and arrived. E.g. did they come as cold interstellar meteors? Or did at least some arrive as hot magma or even more sparse, hot uncondensed cloud-like material?