Condensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites

Details Condensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites Condensation from Cluster-IDP Enriched Vapor Inside the Snow Line: Implications for Mercury, Asteroids, and Enstatite Chondrites

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1797e&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1797

Physics

3

Scientific paper

Cluster-IDPs are a better protoplanetary dust analog than chondritic CI
dust. Condensation with C-IDP enrichments yields silicates with FeO ~0,
plus CaS + MgS above 1000 K. Enstatite chondrites formed inside the snow
line near a C-enriched midplane.

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