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Abstract

The discovery of dwarf planet Eris was followed shortly by the discovery of its satellite, Dysnomia, but the satellite orbit, and thus the system mass, was not known. New observations with the Keck Observatory and the Hubble Space Telescopes show that Dysnomia has a circular orbit with a radius of 37,350 ± 140 (1-σ) kilometers and a 15.774 ± 0.002 day orbital period around Eris. These orbital parameters agree with expectations for a satellite formed out of the orbiting debris left from a giant impact. The mass of Eris from these orbital parameters is 1.67 × 1022 ± 0.02 × 1022 kilograms, or 1.27 ± 0.02 that of Pluto.

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This research is supported by a Presidential Early Career Award to M.E.B. In addition, E.L.S. is supported by a NASA graduate student research fellowship. We thank J. Aycock, R. Campbell, A. Conrad, K. Grace, J. Lyke, C. Melcher, C. Sorenson, M. van Dam, and C. Wilburn at Keck Observatory, without whom these complicated LGS AO observations would not have been possible.

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Published In

Science
Volume 316 | Issue 5831
15 June 2007

Submission history

Received: 29 December 2006
Accepted: 14 March 2007
Published in print: 15 June 2007

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Notes

Supporting Online Material
www.sciencemag.org/cgi/content/full/316/5831/1585/DC1
Materials and Methods
SOM Text
Tables S1 and S1

Authors

Affiliations

Michael E. Brown* [email protected]
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
Emily L. Schaller
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.

Notes

*
To whom correspondence should be addressed. E-mail: [email protected]

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