New Supernova Could Nix Evidence of Dark Matter
An exploding star spotted in 2005 defies the cuurent theories and observations. The theory of how it ignited could explain something unexpected: Why we have calcium in our bones. Astronomers have reported a whole new type of supernova, which seems to spew out calcium and titanium. While most reports focused on the calcium, it's the titanium that's really interesting - the finding could negate ongoing efforts to find signs of dark matter at the center of the Milky Way.
The team of astronomers, led by Hagai Perets, at the Harvard-Smithsonian Center for Astrophysics, and Avishay Gal-Yam of the Weizmann Institute of Science in Rehovot, Israel, presented evidence that supernova SN 2005E is distinct from the two main classes of supernovae: Type Ia supernovae, thought to be old, white dwarf stars that accrete matter from a companion until they undergo a thermonuclear explosion that blows them apart entirely; and Type Ib/c or Type II supernovae, thought to be hot, massive and short-lived stars that explode and leave behind black holes or neutron stars.
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