Cosmic Recipe for Earthlings
By Dolly Setton of Discover Magazine
Stars cook up nearly all of the
approximately 60 atomic elements in people’s bodies. But exactly how that works
remains a mystery. Astrophysicists have developed cutting-edge computer simulations
to grapple with an array of related puzzles:
• What were stars like when they first
appeared in the universe over 13 billion years ago, starting the process of
modern element production?
• What do we know about the nature of
the death of massive stars — signaled by Type II supernovae — that fashion
crucial elements such as calcium and oxygen?
• How might the burned-out stars called
white dwarfs be brought to ruin by other stars in so-called Type Ia supernovae,
inciting the fiery alchemy that yielded much of the iron in our blood and the
potassium in our brains?
Scientists are still trying to figure
out what triggers an individual Type Ia supernova and to determine the identity
of the partner star to the exploding white dwarf. The Hubble Space Telescope’s
recent discovery of the earliest known Type Ia supernova from more than 10
billion years ago, plus other results, favor a scenario in which two white
dwarfs merge.
The results indicate that crucial
elements in people formed later in the history of the universe than many had
expected, says David Jones, the lead astronomer on the Hubble study. “It took
(very roughly) about 750 million years longer to form the first 50 percent of
the iron in the modern universe.”
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