Water Ice on Kuiper Belt Object 1996 TO[TINF]66[/TINF]
Open Access
- 1 July 1999
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 519 (1) , L101-L104
- https://doi.org/10.1086/312098
Abstract
The 1.40-2.45 μm spectrum of Kuiper Belt object 1996 TO66 was measured at the Keck Observatory in 1998 September. Its spectrum shows the strong absorptions near 1.5 and 2.0 μm that are characteristic of water ice—the first such detection on a Kuiper Belt object. The depth of the absorption bands and the continuum reflectance of 1996 TO66 suggest the presence of a black- to slightly blue-colored, spectrally featureless particulate material as a minority component mixed with the water ice. In addition, there is evidence that the intensity of the water bands in the spectrum of 1996 TO66 varies with rotational phase, suggesting a "patchy" surface.Keywords
This publication has 14 references indexed in Scilit:
- The Composition of Centaur 5145 PholusIcarus, 1998
- Identification of Water Ice on the Centaur 1997 CU26Science, 1998
- Surface Composition of Kuiper Belt Object 1993SCScience, 1997
- Stardust MemoriesScience, 1997
- A Search for Slow-Moving Objects and the Luminosity Function of the Kuiper BeltThe Astronomical Journal, 1995
- Dynamical stability in the outer solar system and the delivery of short period cometsThe Astronomical Journal, 1993
- On the fates of minor bodies in the outer solar systemThe Astronomical Journal, 1990
- The origin of short-period cometsThe Astrophysical Journal, 1988
- Temperature dependence of the water-ice spectrum between 1 and 4 microns: Application to Europa, Ganymede and Saturn's ringsIcarus, 1975
- The Origin and Evolution of the Solar SystemMonthly Notices of the Royal Astronomical Society, 1949