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Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion

<!--HTML-->A very close supernova explosion could have caused a mass extinction of life in Earth. In 1996, Brian Fields, the late Dave Schramm and the speaker proposed looking for unstable isotopes such as Iron 60 that could have been deposited by a recent nearby supernova explosion. A group f...

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Autor principal: Ellis, Jonathan R.
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:http://cds.cern.ch/record/2195731
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author Ellis, Jonathan R.
author_facet Ellis, Jonathan R.
author_sort Ellis, Jonathan R.
collection CERN
description <!--HTML-->A very close supernova explosion could have caused a mass extinction of life in Earth. In 1996, Brian Fields, the late Dave Schramm and the speaker proposed looking for unstable isotopes such as Iron 60 that could have been deposited by a recent nearby supernova explosion. A group from the Technical University of Munich has discovered Iron 60 in deep-ocean sediments and ferromanganese crusts due to one or more supernovae that exploded O(100) parsecs away about 2.5 million years ago. These results have recently been confirmed by a group from the Australian National University, and the Munich group has also discovered supernova Iron 60 in lunar rock samples. This talk will discuss the interpretation of these results in terms of supernova models, and the possible implications for life on Earth.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
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spelling cern-21957312022-11-02T22:19:45Zhttp://cds.cern.ch/record/2195731engEllis, Jonathan R.Radioactive Iron Rain: Evidence of a Nearby Supernova ExplosionRadioactive Iron Rain: Evidence of a Nearby Supernova ExplosionCERN Colloquium<!--HTML-->A very close supernova explosion could have caused a mass extinction of life in Earth. In 1996, Brian Fields, the late Dave Schramm and the speaker proposed looking for unstable isotopes such as Iron 60 that could have been deposited by a recent nearby supernova explosion. A group from the Technical University of Munich has discovered Iron 60 in deep-ocean sediments and ferromanganese crusts due to one or more supernovae that exploded O(100) parsecs away about 2.5 million years ago. These results have recently been confirmed by a group from the Australian National University, and the Munich group has also discovered supernova Iron 60 in lunar rock samples. This talk will discuss the interpretation of these results in terms of supernova models, and the possible implications for life on Earth.oai:cds.cern.ch:21957312016
spellingShingle CERN Colloquium
Ellis, Jonathan R.
Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title_full Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title_fullStr Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title_full_unstemmed Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title_short Radioactive Iron Rain: Evidence of a Nearby Supernova Explosion
title_sort radioactive iron rain: evidence of a nearby supernova explosion
topic CERN Colloquium
url http://cds.cern.ch/record/2195731
work_keys_str_mv AT ellisjonathanr radioactiveironrainevidenceofanearbysupernovaexplosion