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Venus' rotation and atmospheric tides

Ingersoll, Andrew P. and Dobrovolskis, Anthony R. (1978) Venus' rotation and atmospheric tides. Nature, 275 . pp. 37-38. ISSN 0028-0836. https://resolver.caltech.edu/CaltechAUTHORS:20130418-080155829

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Abstract

VENUS rotates with a period of 243.00 ± 0.04 d retrograde. The obliquity, or angle between the spin vector and orbit vector is 178 ± 1° (ref. 1). Both the long period and the near 180° obliquity suggest that the spin has evolved under the influence of tidal torques. Tides raised by the Sun in the body of Venus would de-spin the planet in ~10^8 yr if no other torques were acting. The final state would be one of synchronous rotation (one side always facing the Sun). So either we are living during the final stages of Venus' tidal evolution, an unlikely circumstance, or else Venus has already reached a stable equilibrium in which other influences balance the solar body tide. It is possible that the Earth has ‘captured’ Venus into a resonance in which the spin period is 243.165 d. However, for this resonance to be a stable equilibrium, either Venus must have a gravitational field that is ~10 times ‘rougher’ than the Earth's, a possibility that is largely ruled out by direct observation, or a third torque must balance the body torque due to the Sun. Tides in the atmosphere driven by periodic solar heating could supply the necessary third torque, but no quantitative theory has previously been published. Such a theory is presented here, in which we argue that the current rotation is a stable balance between atmospheric and solar body tides.


Item Type:Article
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URLURL TypeDescription
http://dx.doi.org/10.1038/275037a0DOIArticle
http://www.nature.com/nature/journal/v275/n5675/abs/275037a0.htmlPublisherArticle
ORCID:
AuthorORCID
Ingersoll, Andrew P.0000-0002-2035-9198
Additional Information:© 1978 Nature Publishing Group. Received 3 April; accepted 29 June, 1978. This research was supported by NASA.
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Funding AgencyGrant Number
NASAUNSPECIFIED
Record Number:CaltechAUTHORS:20130418-080155829
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130418-080155829
Official Citation:Ingersoll, A. P. and A. R. Dobrovolskis (1978). "Venus' rotation and atmospheric tides." Nature 275(5675): 37-38.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:38007
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:18 Apr 2013 19:06
Last Modified:03 Oct 2019 04:53

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