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An extraterrestrial trigger for the mid-Ordovician ice age: Dust from the breakup of the L-chondrite parent body

Authors :
Schmitz, Birger
Farley, Kenneth A.
Goderis, Steven
Heck, Philipp R.
Bergström, Stig M.
Boschi, Samuele
Claeys, Philippe
Debaille, Vinciane
Dronov, Andrei
van Ginneken, Matthias
Harper, David A.T.
Iqbal, Faisal
Friberg, Johan
Liao, Shiyong
Martin, Ellinor
Meier, Matthias M. M.
Peucker-Ehrenbrink, Bernhard
Soens, Bastien
Wieler, Rainer
Terfelt, Fredrik
Schmitz, Birger
Farley, Kenneth A.
Goderis, Steven
Heck, Philipp R.
Bergström, Stig M.
Boschi, Samuele
Claeys, Philippe
Debaille, Vinciane
Dronov, Andrei
van Ginneken, Matthias
Harper, David A.T.
Iqbal, Faisal
Friberg, Johan
Liao, Shiyong
Martin, Ellinor
Meier, Matthias M. M.
Peucker-Ehrenbrink, Bernhard
Soens, Bastien
Wieler, Rainer
Terfelt, Fredrik
Publication Year :
2019

Abstract

The breakup of the L-chondrite parent body in the asteroid belt 466 million years (Ma) ago still delivers almost a third of all meteorites falling on Earth. Our new extraterrestrial chromite and 3He data for Ordovician sediments show that the breakup took place just at the onset of a major, eustatic sea level fall previously attributed to an Ordovician ice age. Shortly after the breakup, the flux to Earth of the most fine-grained, extraterrestrial material increased by three to four orders of magnitude. In the present stratosphere, extraterrestrial dust represents 1% of all the dust and has no climatic significance. Extraordinary amounts of dust in the entire inner solar system during >2 Ma following the L-chondrite breakup cooled Earth and triggered Ordovician icehouse conditions, sea level fall, and major faunal turnovers related to the Great Ordovician Biodiversification Event.

Details

Database :
OAIster
Notes :
application/pdf, An extraterrestrial trigger for the mid-Ordovician ice age: Dust from the breakup of the L-chondrite parent body, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1258096615
Document Type :
Electronic Resource