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Published Online March 6, 2003
Science DOI: 10.1126/science.1079645

Research Articles

Submitted on October 22, 2002
Accepted on February 19, 2003

Fluid Core Size of Mars from Detection of the Solar Tide

C. F. Yoder 1*, A. S. Konopliv 2*, D. N. Yuan 2, E. M. Standish 1, W. M. Folkner 2

1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

* To whom correspondence should be addressed. E-mail: Charles.F.Yoder{at}jpl.nasa.gov, Alex.konopliv{at}jpl.nasa.gov.

The solar tidal deformation of Mars, measured by its k2 potential Love number, has been obtained from analysis of Mars Global Surveyor radio tracking. The observed k2 = 0.153 ± 0.017 is large enough to rule out a solid iron core and so indicates that at least the outer part of the core is liquid. The inferred core radius Rc (1520km< Rc <1840km) is independent of many interior properties, although partial melt of the mantle is one factor that could reduce core size. Ice cap mass changes can be deduced from the seasonal variations in air pressure and the odd gravity harmonic J3, given knowledge of cap mass distribution with latitude. The south cap seasonal mass change is about 30 to 40% larger than the north cap.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Mars: A New Core-Crystallization Regime.
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Science 316, 1323-1325
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New Perspectives on Ancient Mars.
S. C. Solomon, O. Aharonson, J. M. Aurnou, W. B. Banerdt, M. H. Carr, A. J. Dombard, H. V. Frey, M. P. Golombek, S. A. Hauck II, J. W. Head III, et al. (2005)
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Thermal evolution of the Martian core: Implications for an early dynamo.
(2004)
Geology 32, 97-100



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Science. ISSN 0036-8075 (print), 1095-9203 (online)