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Water Ice on the Satellite of Kuiper Belt Object 2003 EL61

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arxiv astro-ph/0601534 v1 pith:LSXXODK6 submitted 2006-01-24 astro-ph

classification astro-ph
keywords satellitebeltkuiperspectrumwaterabsorptionel61features
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We have obtained a near infrared spectrum of the brightest satellite of the large Kuiper Belt Object, 2003 EL61. The spectrum has absorption features at 1.5 and 2.0 microns, indicating that water ice is present on the surface. We find that the satellite's absorption lines are much deeper than water ice features typically found on Kuiper Belt Objects. We argue that the unusual spectrum indicates that the satellite was likely formed by impact and not by capture.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Beyond Point Masses. VI. Spin-Orbit Evolution of the Centaur Binary Typhon-Echidna

    astro-ph.EP 2026-08 conditional novelty 6.0 of 10

    The mutual orbit of Typhon-Echidna is precessing rapidly, revealing Typhon's J2, a 24 degree spin-orbit misalignment, and a triaxial shape consistent with a recently excited binary.

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