Long term behavior of a hypothetical planet in a highly eccentric orbit

Details Long term behavior of a hypothetical planet in a highly eccentric orbit Long term behavior of a hypothetical planet in a highly eccentric orbit

1999-09-28

arxiv.org/abs/astro-ph/9909464v1

Astronomy and Astrophysics

Astrophysics

8 pages, 5 figures, LaTeX

Scientific paper

For a hypothetical planet on a highly eccentric orbit, we have calculated the
osculating orbital parameters and its closest approaches to Earth and Moon over
a period of 750 kyr. The approaches which are close enough to influence the
climate of the Earth form a pattern comparable to that of the past climatic
changes, as recorded in deep sea sediments and polar ice cores.

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