Roe, Henry G. and Pike, Rosemary E. and Brown, Michael E. (2008) Tentative detection of the rotation of Eris. Icarus, 198 (2). pp. 459-464. ISSN 0019-1035. doi:10.1016/j.icarus.2008.08.001. https://resolver.caltech.edu/CaltechAUTHORS:ROEica08
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Abstract
We report a multi-week sequence of B-band photometric measurements of the dwarf planet Eris using the Swift satellite. The use of an observatory in low-Earth orbit provides better temporal sampling than is available with a ground-based telescope. We find no compelling evidence for an unusually slow rotation period of multiple days, as has been suggested previously. A not, vert, similar1.08 day rotation period is marginally detected at a modest level of statistical confidence (~97%). Analysis of the combination of the Swift data with the ground-based B-band measurements of Rabinowitz et al. [Rabinowitz, D.L., Schaefer, B.E., Tourtellotte, S.W., 2007. Astron. J. 133, 26–43] returns the same period (~1.08 day) at a slightly higher statistical confidence (~99%).
Item Type: | Article | |||||||||
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Additional Information: | © 2008 Elsevier. Received 30 April 2008; revised 28 July 2008. Available online 4 September 2008. We thank David Rabinowitz and an anonymous referee. | |||||||||
Subject Keywords: | Kuiper belt | |||||||||
Issue or Number: | 2 | |||||||||
DOI: | 10.1016/j.icarus.2008.08.001 | |||||||||
Record Number: | CaltechAUTHORS:ROEica08 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:ROEica08 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 12934 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | Archive Administrator | |||||||||
Deposited On: | 11 Jan 2009 04:27 | |||||||||
Last Modified: | 08 Nov 2021 22:34 |
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