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Volumn 336, Issue 6082, 2012, Pages 687-690

Vesta's shape and morphology

(43)  Jaumann, R a,b   Williams, D A c   Buczkowski, D L d   Yingst, R A e   Preusker, F a   Hiesinger, H f   Schmedemann, N b   Kneissl, T b   Vincent, J B g   Blewett, D T d   Buratti, B J h   Carsenty, U a   Denevi, B W d   De Sanctis, M C i   Garry, W B e   Keller, H U j   Kersten, E a   Krohn, K a   Li, J Y k   Marchi, S l   more..


Author keywords

[No Author keywords available]

Indexed keywords

ASTEROID; BEDROCK; CRATER; MASS WASTING; MOON; PLANET; REGOLITH; SHAPE; SOLAR SYSTEM;

EID: 84860826008     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1219122     Document Type: Article
Times cited : (208)

References (20)
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    • Methods and additional materials are available as supplementary materials on
    • Methods and additional materials are available as supplementary materials on Science Online.
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    • (2012) Science , vol.336 , pp. 690
    • Marchi, S.1
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    • (1996) Icarus , vol.120 , pp. 158
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  • 13
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    • thesis, UCLA, Los Angeles, CA
    • B. E. Schmidt, thesis, UCLA, Los Angeles, CA (2011).
    • (2011)
    • Schmidt, B.E.1
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    • note
    • The error on ejecta thickness is estimated by multiplying the crater depth-to-diameter ratio with the bin width (500 m) of the crater sizes at which the slope of the crater frequency distribution curve is changing because of resurfacing (fig. S1).
  • 15
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    • A. F. Cheng et al., Icarus 155, 51 (2002).
    • (2002) Icarus , vol.155 , pp. 51
    • Cheng, A.F.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.