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Volumn 330, Issue 6006, 2010, Pages 949-951

Structure and formation of the lunar farside highlands

Author keywords

[No Author keywords available]

Indexed keywords

CRUSTAL THICKNESS; HARMONIC ANALYSIS; HEAT PRODUCTION; LUNAR CRUST; MAGMA; MOON; SPATIAL VARIATION; TERRAIN; TOPOGRAPHY; VOLCANISM;

EID: 78149389148     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1193424     Document Type: Article
Times cited : (43)

References (30)
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    • J. A. Wood, Moon 8, 73 (1973).
    • (1973) Moon , vol.8 , pp. 73
    • Wood, J.A.1
  • 9
    • 60149103305 scopus 로고    scopus 로고
    • N. Namiki et al., Science 323, 900 (2009).
    • (2009) Science , vol.323 , pp. 900
    • Namiki, N.1
  • 17
    • 0003833228 scopus 로고
    • Cambridge Univ. Press, Cambridge
    • H. Jeffreys, The Earth (Cambridge Univ. Press, Cambridge, 1976).
    • (1976) The Earth
    • Jeffreys, H.1
  • 25
    • 78149365656 scopus 로고    scopus 로고
    • note
    • Crustal-thickness differences may also be lowered as the remaining liquids under the crust crystallize (SOM section 8).
  • 27
    • 78149369838 scopus 로고    scopus 로고
    • note
    • We have multiplied the actual crustal thickness by 0.4 to better match the thickness amplitudes in the two cases.
  • 30
    • 78149402565 scopus 로고    scopus 로고
    • note
    • We thank E. M. Parmentier, G. Hirth, L. Elkins-Tanton, M. T. Zuber, J. Andrews-Hanna, G. A. Glatzmaier, P. C. Hess, and M. J. Rutherford for helpful discussions. This work was made possible by a Brown University postdoctoral research assistantship to I.G.-B.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.