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Volumn 314, Issue 5806, 2006, Pages 1711-1716

Comet 81P/wild 2 under a microscope

(183)  Brownlee, Don a   Tsou, Peter b   Aléon, Jérôme c,d   O'D Alexander, Conel M e   Araki, Tohru f   Bajt, Sasa d   Baratta, Giuseppe A g   Bastien, Ron h   Bland, Phil i,j   Bleuet, Pierre k   Borg, Janet l   Bradley, John P m   Brearley, Adrian n   Brenker, F o   Brennan, Sean p   Bridges, John C q   Browning, Nigel D d,r   Brucato, John R s   Bullock, E t   Burchell, Mark J u   more..


Author keywords

[No Author keywords available]

Indexed keywords

ELEMENTARY PARTICLES; HIGH TEMPERATURE APPLICATIONS; MATHEMATICAL MODELS; MICROSCOPES; SILICATE MINERALS; SOLAR SYSTEM; SPACECRAFT;

EID: 33845685034     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1135840     Document Type: Article
Times cited : (836)

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    • note
    • Unequilibrated meteoritic materials have not experienced substantial diffusion of atoms between components, usually due to heating, that causes phases such as olivine to have the same elemental composition. The wide range of Fe/Mg ratios in Wild 2 olivine as well as the Ni content of Sulfides show that the comet is at least as unequilibrated as the very rare and least equilibrated meteorites.
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    • note
    • The Stardust sample analysis team is grateful to NASA for funding and supporting the mission and to the hundreds of other team members that were involved in design, construction, flying, and recovery of the mission. The team, from 100 organizations, gratefully acknowledges their supporting institutions.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.