Processing of refractory meteorite inclusions (CAIs) in parent-body atmospheres

  • Morris Podolak*
  • , T. E. Bunch
  • , Pat Cassen
  • , Ray T. Reynolds
  • , S. Chang
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

The refractory meteorite inclusions known as CAIs (calcium-aluminum rich inclusions) display melted rims that were produced by thermal events of only a few seconds duration. We show that gas dynamic deceleration in a temporary atmosphere around an accreting parent body, produced by gas release during accretion, could provide a regime of sufficiently high gas density and small scale height to achieve partial melting of the CAIs. In addition, the presence of dust in the atmosphere would increase the gradient of pressure with height (i.e., effectively reduce the scale height), lower the rate of blowoff (thus keeping more gas around the body), as well as allow dust particles to become trapped in the partially melted material as is observed in some cases. Thus, CAIs may be regarded as probes of a primitive atmosphere by virtue of the thermal and mineralogical alteration that occurred upon their passage through the atmosphere.

Original languageEnglish
Pages (from-to)254-260
Number of pages7
JournalIcarus
Volume84
Issue number1
DOIs
StatePublished - Mar 1990
Externally publishedYes

Funding

Funders
National Aeronautics and Space Administration Planetary Geosciences, Planetary Mate° rials and Geochemistry, and Life Sciences Exobiology Programs

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