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Volumn 44, Issue 5, 1996, Pages 427-430

Evolution of the earth obliquity after the tidal expansion of the moon orbit

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EID: 30244487227     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(95)00157-3     Document Type: Article
Times cited : (9)

References (13)
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  • 6
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    • The chaotic motion of the Solar System: A numerical estimate of the size of the chaotic zones
    • Laskar, J., The chaotic motion of the Solar System: a numerical estimate of the size of the chaotic zones. Icarus 88, 266, 1990.
    • (1990) Icarus , vol.88 , pp. 266
    • Laskar, J.1
  • 7
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    • The chaotic obliquity of the planets
    • Laskar, J. and Robutel, R., The chaotic obliquity of the planets. Nature 361, 608, 1993.
    • (1993) Nature , vol.361 , pp. 608
    • Laskar, J.1    Robutel, R.2
  • 8
    • 0027455839 scopus 로고
    • Stabilization of the Earth's obliquity by the Moon
    • Laskar, J., Joutel, R. and Robutel, R., Stabilization of the Earth's obliquity by the Moon. Nature 361, 615, 1993.
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  • 9
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    • Seasoned travellers
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    • Climatic variations on Mars 1. Astronomical theory of insulation
    • Ward, W. R., Climatic variations on Mars 1. Astronomical theory of insulation. J. Geophys. Res. 79, 3375, 1974.
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  • 11
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    • Present obliquity oscillations of Mars: Fourth-order accuracy in orbital e and I
    • Ward, W. R., Present obliquity oscillations of Mars: fourth-order accuracy in orbital e and I. J. Geophys. Res. 84, 237, 1979.
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    • Long-term orbital and spin dynamics of Mars
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    • Ward, W. R., Long-term orbital and spin dynamics of Mars, in Mars (edited by H. H. Kieffer, B. M. Jakosky, C. W. Snyder and M. S. Matthews), p. 298. The University of Arizona Press, Tucson, 1992.
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    • Ward, W.R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.