Amalthea's Density Is Less Than That of Water

Author:

Anderson John D.12345,Johnson Torrence V.12345,Schubert Gerald12345,Asmar Sami12345,Jacobson Robert A.12345,Johnston Douglas12345,Lau Eunice L.12345,Lewis George12345,Moore William B.12345,Taylor Anthony12345,Thomas Peter C.12345,Weinwurm Gudrun12345

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109-8099, USA.

2. Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA.

3. Institute of Geophysics and Planetary Physics, Los Angeles, CA 90095-1567, USA.

4. Center for Radio Physics and Space Research, Cornell University, Ithaca, NY 14853-4901, USA.

5. Institute of Geodesy and Geophysics, Vienna University of Technology, A-1040 Vienna, Austria.

Abstract

Radio Doppler data from the Galileo spacecraft's encounter with Amalthea, one of Jupiter's small inner moons, on 5 November 2002 yield a mass of (2.08 ± 0.15) × 10 18 kilograms. Images of Amalthea from two Voyager spacecraft in 1979 and Galileo imaging between November 1996 and June 1997 yield a volume of (2.43 ± 0.22) × 10 6 cubic kilometers. The satellite thus has a density of 857 ± 99 kilograms per cubic meter. We suggest that Amalthea is porous and composed of water ice, as well as rocky material, and thus formed in a cold region of the solar system, possibly not at its present location near Jupiter.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference24 articles.

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2. D. J. Tholen, V. G. Tejfel, A. N. Cox, in Allen's Astrophysical Quantities Fourth Edition, A. N. Cox, Ed. (Springer-Verlag, New York, 2000), pp. 302-310.

3. D. C. Jewitt, G. E. Danielson, S. P. Synnott, Science206, 951 (1979).

4. 1979J2: The Discovery of a Previously Unknown Jovian Satellite

5. S. P. Synnott, Science210, 1392 (1980).

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