| Literature DB >> 17732249 |
Abstract
Numerical integration of the rotation of Mars shows that the obliquity of Mars undergoes large chaotic variations. These variations occur as the system evolves in the chaotic zone associated with a secular spin-orbit resonance.Year: 1993 PMID: 17732249 DOI: 10.1126/science.259.5099.1294
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728