Late Precambrian paradoxical glaciation and obliquity of the Earth -: a discussion of dynamical constraints

被引:22
|
作者
Pais, MA
Le Mouël, JL
Lambeck, K
Poirier, JP
机构
[1] Inst Phys Globe, Lab Geomagnetisme, F-75252 Paris 05, France
[2] Australian Natl Univ, Res Sch Earth Sci, Canberra, ACT 0200, Australia
[3] Inst Phys Globe, Lab Geomat, F-75252 Paris 05, France
关键词
paleoclimatology; rotation; precession; obliquity of the ecliptic; core-mantle boundary;
D O I
10.1016/S0012-821X(99)00249-6
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
G.E, Williams' observations on Late Precambrian glaciogenic sequences pose some major challenges to the understanding of the dynamical evolution of the Earth's orbit and spin that have not yet been adequately addressed. In this paper, we investigate whether dissipative core-mantle coupling is an effective mechanism for reducing the obliquity by such a large amount as suggested by Williams [G.E. Williams, Earth Sci, Rev. 112 (1993) 1-45], and we examine the relationship between the obliquity and spin rate in the presence of such coupling. We show that this mechanism not only cannot explain the rapid and substantial decrease in obliquity, but also that such a decrease is in contradiction with existing paleorotation evidence for the same period, thus confirming the previous findings of Ni ron de Surgy and Laskar [O. Neron de Surgy, J. Laskar, Astron. Astrophys. 318 (1997) 975-989]. (C) 1999 Elsevier Science B.V. All rights reserved.
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页码:155 / 171
页数:17
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