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The neutron star.Ingredients: One large, well matured star (As small as 8 solar masses to 20 solar masses) That's it....Method: Turn up heat to 100 million Kevin. This allows Helium and other heavier elements to begin fusion, bringing the more complex elements in the dish to the fore. Reduce the mixture for around a million years. Now you should see characteristic "onion" layers forming, with light hydrogen on the outer shell getting denser and chewy towards the iron, inner core. At this stage … -
I have no idea how much 1 kevin is but your examples are very funny. Look it up on wikipedia or somethng. It might not even be real. It's hard to choose a tempereture that is hotter than everything in oure solar system that is hot together. What ever I just said... Just confused me more.
