Low-latitude glaciation and rapid changes in the Earth's obliquity explained by obliquity–oblateness feedback

Darren M. Williams (), James F. Kasting and Lawrence A. Frakes
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Darren M. Williams: School of Science, Penn State Erie, The Behrend College
James F. Kasting: The Pennsylvania State University, 443 Deike Building, University Park
Lawrence A. Frakes: University of Adelaide

Nature, 1998, vol. 396, issue 6710, 453-455

Abstract: Abstract Palaeomagnetic data suggest that the Earth was glaciated at low latitudes during the Palaeoproterozoic1,2 (about 2.4–2.2 Gyr ago) and Neoproterozoic3,4,5,6,7,8 (about 820–550 Myr ago) eras, although some of the Neoproterozoic data are disputed9,10. If the Earth's magnetic field was aligned more or less with its spin axis, as it is today, then either the polar ice caps must have extended well down into the tropics — the ‘snowball Earth’ hypothesis8 — or the present zonation of climate with respect to latitude must have been reversed. Williams11 has suggested that the Earth's obliquity may have been greater than 54° during most of its history, which would have made the Equator the coldest part of the planet12. But this would require a mechanism to bring the obliquity down to its present value of 23.5°. Here we propose that obliquity–oblateness feedback13 could have reduced the Earth's obliquity by tens of degrees in less than 100 Myr if the continents were situated so as to promote the formation of large polar ice sheets. A high obliquity for the early Earth may also provide a natural explanation for the present inclination of the lunar orbit with respect to the ecliptic (5°), which is otherwise difficult to explain.

Date: 1998
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DOI: 10.1038/24845

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