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Large-scale thermal events in the solar nebula: evidence from Fe,Ni metal grains in primitive meteorites | A Meibom
; S J Desch
; A N Krot
; J N Cuzzi
; M I Petaev
; L Wilson
; K Keil
; | Date: |
5 May 2000 | Journal: | Science, 288 (5467), 839-41 | Abstract: | Chemical zoning patterns in some iron, nickel metal grains from CH carbonaceous chondrites imply formation at temperatures from 1370 to 1270 kelvin by condensation from a solar nebular gas cooling at a rate of approximately 0.2 kelvin per hour. This cooling rate requires a large-scale thermal event in the nebula, in contrast to the localized, transient heating events inferred for chondrule formation. In our model, mass accretion through the protoplanetary disk caused large-scale evaporation of precursor dust near its midplane inside of a few astronomical units. Gas convectively moved from the midplane to cooler regions above it, and the metal grains condensed in these parcels of rising gas. | Source: | PubMed, pmid10797001 doi: 8501 | Services: | Forum | Review | Favorites |
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