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

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dc.creatorNufer, R.
dc.creatorBaltensperger, W.
dc.creatorWoelfli, W.
dc.date1999-09-28
dc.date.accessioned2026-07-07T02:33:31Z
dc.date.available2026-07-07T02:33:31Z
dc.descriptionFor 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.
dc.description8 pages, 5 figures, LaTeX
dc.identifierhttps://arxiv.org/abs/astro-ph/9909464
dc.identifierhttp://arxiv.org/abs/astro-ph/9909464
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14874
dc.subjectAstrophysics
dc.titleLong term behavior of a hypothetical planet in a highly eccentric orbit
dc.typetext

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