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Organics in meteorites - Solar or interstellar?

Published online by Cambridge University Press:  01 February 2008

Conel M. O'D. Alexander ,
George D. Cody ,
Marilyn Fogel  and
Hikaru Yabuta
Conel M. O'D. Alexander
Affiliation:
DTM, Carnegie Institution of Washington, 5241 Broad Branch Road, Washington DC 20015, USA email: alexande@dtm.ciw.edu
George D. Cody
Affiliation:
GL, Carnegie Institution of Washington, 5251 Broad Branch Road, Washington DC 20015, USA email: g.cody@gl.ciw.edu, m.fogel@gl.ciw.edu, hyabuta@gl.ciw.edu
Marilyn Fogel
Affiliation:
GL, Carnegie Institution of Washington, 5251 Broad Branch Road, Washington DC 20015, USA email: g.cody@gl.ciw.edu, m.fogel@gl.ciw.edu, hyabuta@gl.ciw.edu
Hikaru Yabuta
Affiliation:
GL, Carnegie Institution of Washington, 5251 Broad Branch Road, Washington DC 20015, USA email: g.cody@gl.ciw.edu, m.fogel@gl.ciw.edu, hyabuta@gl.ciw.edu
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Abstract

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The insoluble organic material (IOM) in primitive meteorites is related to the organic material in interplanetary dust particles and comets, and is probably related to the refractory organic material in the diffuse interstellar medium. If the IOM is representative of refractory ISM organics, models for how and from what it formed will have to be revised.

Keywords

CometsasteroidsISM: dust
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S251: Organic Matter in Space , February 2008 , pp. 293 - 298
Copyright
Copyright © International Astronomical Union 2008

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