Identification of Water Ice on the Centaur 1997 CU26
- 29 May 1998
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 280 (5368) , 1430-1432
- https://doi.org/10.1126/science.280.5368.1430
Abstract
Spectra of the Centaur 1997 CU26 were obtained at the Keck Observatory on 27 October 1997 (universal time). The data show strong absorptions at 1.52 and 2.03 micrometers attributable to water ice on the surface of 1997 CU26. The reflectance spectrum of 1997 CU26 is matched by the spectrum of a mixture of low-temperature, particulate water ice and spectrally featureless but otherwise red-colored material. Water ice dominates the spectrum of 1997 CU26, whereas methane or methane-like hydrocarbons apparently dominate the spectrum of the Kuiper belt object 1993 SC, perhaps indicating different origins, thermal histories, or both for these two objects.Keywords
This publication has 8 references indexed in Scilit:
- Optical and Infrared Reflectance Spectrum of Kuiper Belt Object 1996 TL[TINF]66[/TINF]The Astrophysical Journal, 1998
- Surface Composition of Kuiper Belt Object 1993SCScience, 1997
- The Mauna Kea-Cerro-Tololo (MKCT) Kuiper Belt and Centaur SurveyThe Astronomical Journal, 1996
- Infrared optical constants of H2O ice, amorphous nitric acid solutions, and nitric acid hydratesJournal of Geophysical Research: Atmospheres, 1994
- Near-Infrared Spectroscopy of Primitive Solar System ObjectsIcarus, 1994
- Optical constants of ice from the ultraviolet to the microwaveApplied Optics, 1984
- THE INFRARED SPECTRAL PROPERTIES OF FROZEN VOLATILESPublished by JSTOR ,1982
- The Origin and Evolution of the Solar SystemMonthly Notices of the Royal Astronomical Society, 1949