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Volumn 336, Issue 6082, 2012, Pages 684-686

Dawn at vesta: Testing the protoplanetary paradigm

(28)  Russell, C T a   Raymond, C A b   Coradini, A c   McSween, H Y d   Zuber, M T e   Nathues, A f   De Sanctis, M C c   Jaumann, R g   Konopliv, A S b   Preusker, F g   Asmar, S W b   Park, R S b   Gaskell, R i   Keller, H U f   Mottola, S g   Roatsch, T g   Scully, J E C h   Smith, D E e   Tricarico, P i   Toplis, M J j   more..


Author keywords

[No Author keywords available]

Indexed keywords

DIOGENITE; EUCRITE; EXCAVATION; GRAVITY FIELD; HOWARDITE; IRON; MINERALOGY; PREDICTION; SOLAR SYSTEM; SPACECRAFT;

EID: 84860806312     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1219381     Document Type: Article
Times cited : (453)

References (32)
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    • note
    • Vesta's volume was estimated using three methods: (1) a stereophotoclinometrically derived (SPC) shape model that filled in the unmeasured northern latitudes with spherical harmonics fit to the measured region; (2) the SPC shape model that used the Thomas shape model (11) to fill in the northern cap; and (3) the stereophotogrammetrically derived shape model filled in the north with the SPC harmonics. The differences were 0.28% between models 1 and 2 and 0.059% between 1 and 3, indicating that the unmeasured northern cap is unlikely to cause a large uncertainty in the volume estimate. Model 2 is used throughout this report.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.