Not exact matches
Co-author Daniel Kasen from UC Berkeley and Lawrence Berkeley National Lab created models of the
supernova that explained the data as the explosion of a star only a few times the size of the sun and rich
in carbon and
oxygen.
«The
oxygen we breathe, the iron
in our blood, the carbon
in plants, the silicon
in the sand — all the matter that makes up you and the Earth is made and distributed by
supernovae,» Janka says.
And physicists are using computer modeling to close
in on the neutrino's critical role
in triggering the kind of
supernovae that distribute essential elements like
oxygen and nitrogen.
The
oxygen - rich
supernova dust grain has a different composition than one reported earlier this year
in Nature by cosmochemist Larry Nittler of the Carnegie Institution
in Washington, D.C. «That's exciting,» says Nittler.
The amount of
oxygen in a galaxy is determined primarily by three factors: how much
oxygen comes from large stars that end their lives violently
in supernova explosions — a ubiquitous phenomenon
in the early Universe, when the rate of stellar births was dramatically higher than the rate
in the Universe today; how much of that
oxygen gets ejected from the galaxy by so - called «super winds,» which propel
oxygen and other interstellar gases out of galaxies at hundreds of thousands of miles per hour; and how much pristine gas enters the galaxy from the intergalactic medium, which doesn't contain much
oxygen.