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Science
Volumn 248, Issue 4956, 1990, Pages 720-721
Mars: Change in axial tilt due to climate?
Author keywords

[No Author keywords available]
Indexed keywords

AXIAL TILT; CLIMATIC VARIATION; EFFECTIVE VISCOSITY; MASS DISTRIBUTION; OBLIQUITY; SOLAR TORQUE;
EID: 0025243289     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.248.4956.720     Document Type: Article
Times cited : (29)
References (18)
  • 6
    • 85027749244 scopus 로고    scopus 로고
    • paper presented at the annual spring meeting of the American Geophysical Union, Baltimore, MD, 7 to 12 May 1989. Bills has the average obliquity having a value as high as 40° only tens of millions of years ago. His model depends on a value of the moment of inertia that is substantially smaller than the accepted value.
    • Bills, B.G.1
  • 14
    • 84994998684 scopus 로고
    • 2 is removed uniformly all over the regolith and deposited evenly on the cap. D. P. Rubincam [J. Geophys. Res. 89, 1077 (1984)] considers a similar case for the oceans and the Laurentide ice sheet on Earth, but with the more sophisticated layered model of P. Wu and W. R. Peltier [Geophys. J. R. Astron. Soc. 70,435 (1982)]. The simple model adopted here can only give orders of magnitude for viscosities.
    • (1974) Rev. Geophys. Space Phys. , vol.12 , pp. 649
    • Peltier, W.R.1

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.