Large-scale thermal events in the solar nebula: Evidence from Fe,Ni metal grains in primitive meteorites

Science

Volumn 288, Issue 5467, 2000, Pages 839-841

  Meibom, Anders ^a,f   Desch, Steven J ^b   Krot, Alexander N ^a   Cuzzi, Jeffrey N ^b   Petaev, Michael I ^c   Wilson, Lionel ^d   Keil, Klaus ^a,e  

^a UNIVERSITY OF HAWAII   (United States)

^b NASA AMES RESEARCH CENTER   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d LANCASTER UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF HAWAII   (United States)

^f STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

IRON; NICKEL;

CARBONACEOUS CHONDRITE; CHONDRITE; IRON; METEORITE; NICKEL;

ARTICLE; ASTRONOMY; CRYSTALLIZATION; EVAPORATION; HEATING; KINETICS; NONHUMAN; PRECURSOR; PRIORITY JOURNAL; THERMODYNAMICS;

EID: 0034607815     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.288.5467.839     Document Type: Article

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31. This collaboration between meteoriticists and astrophysicists was spurred by the 1999 Gordon Research Conference (Origins of Solar Systems), which brought together researchers from both disciplines in a highly inspiring scientific environment. Our work was supported by NASA grants 5-4212 (K. Keil, P.I.) and NAGW 3451 (J. A. Wood, P.I.) and NASA's Origins of Solar Systems program (J. Cuzzi, P.I.). A.M. is grateful for support from the Danish Natural Science Research Council S.J.D. was supported by a National Research Council Research Associateship. We appreciate illuminating discussions with R. Bell, H. Klahr, A. Showman, A. Luntz, F. Besenbacher, T. Fagan, E. Scott, and J. Taylor.