| | |  | | | | Record from Web of Science® | |  |  | | |  |
| STABILIZATION OF THE EARTHS OBLIQUITY BY THE MOON |
|
|
| Author(s): LASKAR J, JOUTEL F, ROBUTEL P |
| Source: NATURE Volume: 361 Issue: 6413 Pages: 615-617 Published: FEB 18 1993 |
| Times Cited: 100 References: 14 |
| Abstract: 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. |
| Document Type: Article |
| Language: English |
| Reprint Address: LASKAR, J (reprint author), BUR LONGITUDES, 77 AVE DENFERT ROCHEREAU, F-75014 PARIS, FRANCE |
| Publisher: MACMILLAN MAGAZINES LTD, PORTERS SOUTH, 4 CRINAN ST, LONDON, ENGLAND N1 9XW |
| Subject Category: Multidisciplinary Sciences |
| IDS Number: KM776 |
| ISSN: 0028-0836 |
|
| |  |  |  |  | | | | Record from Web of Science® | |  |  | | | | | | |