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The Multiple Origins of Insoluble Organic Matter from Primitive Chondrites

E. Quirico 1 F.-R. Orthous-Daunay 1 L. Bonal 1 P. Beck 1 R. Brunetto 2 E. Dartois 2 T. Pino 3 C. Engrand 4 J. Duprat
1 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
2 IAS - Institut d'astrophysique spatiale
3 ISMO - Institut des Sciences Moléculaires d'Orsay
4 CSNSM AS
CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse
Abstract : We present a study by IR and Raman of the insoluble organic matter from 28 CI, CR, CM and ung-C2 chondrites. We evidence a chemical heterogeneity of the solar nebula and that thermal heating was the sole parent body process that modified IOM.
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Conference papers
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http://hal.in2p3.fr/in2p3-00780146
Contributor : Christine Hadrossek <>
Submitted on : Monday, January 28, 2013 - 12:15:19 PM
Last modification on : Monday, January 4, 2021 - 9:30:03 AM

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E. Quirico, F.-R. Orthous-Daunay, L. Bonal, P. Beck, R. Brunetto, et al.. The Multiple Origins of Insoluble Organic Matter from Primitive Chondrites. Asteroids, Comets, Meteors 2012, 2012, Niigata, Japan. ⟨in2p3-00780146⟩

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