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Chemical evolution of planetary materials in a dynamic solar nebula

Published online by Cambridge University Press:  12 October 2020

Fred J. Ciesla Open the ORCID record for Fred J. Ciesla [Opens in a new window]
Fred J. Ciesla*
Affiliation:
Department of the Geophysical Sciences, The University of Chicago, Chicago, IL60615, USA email: fciesla@uchicago.edu
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Abstract

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As observational facilities improve, providing new insights into the chemistry occurring in protoplanetary disks, it is important to develop more complete pictures of the processes that shapes the chemical evolution of materials during this stage of planet formation. Here we describe how primitive meteorites in our own Solar System can provide insights into the processes that shaped planetary materials early in their evolution around the Sun. In particular, we show how this leads us to expect protoplanetary disks to be very dynamic objects and what modeling and laboratory studies are needed to provide a more complete picture for the early chemical evolution that occurs for planetary systems.

Keywords

planetary systems: formationplanetary systems: protoplanetary disksplanets and satellites: formationsolar system: formationcomets: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S350: Laboratory Astrophysics: From Observations to Interpretation , April 2019 , pp. 152 - 157
Copyright
© International Astronomical Union 2020

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