THE SURFACE COMPOSITION OF LARGE KUIPER BELT OBJECT 2007 OR10
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Brown-2011-THE SURFACE COMPOSIT.pdf
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Author(s)
Brown, M. E.
Burgasser, Adam J.
Fraser, W. C.
Date Issued
September 2011
Journal
Astrophysical Journal
Publisher
Institute of Physics/American Astronomical Society
Citation
Brown, M. E., A. J. Burgasser, and W. C. Fraser. “THE SURFACE COMPOSITION OF LARGE KUIPER BELT OBJECT 2007 OR10.” The Astrophysical Journal 738, no. 2 (August 22, 2011): L26. © 2011 American Astronomical Society.
Version
Final published version
Abstract
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice. While most objects in the Kuiper belt with water ice absorption this prominent have the optically neutral colors of water ice, 2007 OR10 is among the reddest Kuiper belt objects known. One other large Kuiper belt object—Quaoar—has similar red coloring and water ice absorption, and it is hypothesized that the red coloration of this object is due to irradiation of the small amounts of methane able to be retained on Quaoar. 2007 OR10, though warmer than Quaoar, is in a similar volatile retention regime because it is sufficiently larger that its stronger gravity can still retain methane. We propose, therefore, that the red coloration on 2007 OR10 is also caused by the retention of small amounts of methane. Positive detection of methane on 2007 OR10 will require spectra with higher signal to noise. Models for volatile retention on Kuiper belt objects appear to continue to do an excellent job reproducing all of the available observations.
MIT Department
Massachusetts Institute of Technology. Department of Physics
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
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DOI of Published Version
https://doi.org/10.1088/2041-8205/738/2/l26
