STABILIZATION OF THE EARTHS OBLIQUITY BY THE MOON

被引:220
作者
LASKAR, J
JOUTEL, F
ROBUTEL, P
机构
[1] Astronomie et Systèmes Dynamiques, Bureau des Longitudes, F75014 Paris
关键词
D O I
10.1038/361615a0
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
ACCORDING to Milankovitch theory1,2, the ice ages are related to variations of insolation in northern latitudes resulting from changes in the Earth's orbital and orientation parameters (precession, eccentricity and obliquity). Here we investigate the stability of the Earth's orientation for all possible values of the initial obliquity, by integrating the equations of precession of the Earth. We find a large chaotic zone which extends from 60-degrees to 90-degrees in obliquity. In its present state, the Earth avoids this chaotic zone and its obliquity is essentially stable, exhibiting only small variations of +/- 1.3-degrees around the mean value of 23.3-degrees. But if the Moon were not present, the torque exerted on the Earth would be smaller, and the chaotic zone would then extend from nearly 0-degrees up to about 85-degrees. Thus, had the planet not acquired the Moon, large variations in obliquity resulting from its chaotic behaviour might have driven dramatic changes in climate. In this sense one might consider the Moon to act as a potential climate regulator for the Earth.
引用
收藏
页码:615 / 617
页数:3
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