and special conditions in the surface microstructure may affect the spectroscopic signature of water ice in such a way that crystalline ice is present and its 1.65 ยตm spectral band is masked. Our spectra (1.87-2.5 ยตm) taken at an interval of nearly 3.5 years do not show any significant changes that
Water Ice on Nereid
โ Scribed by Robert H. Brown; Dale P. Cruikshank; Yvonne Pendleton; Glenn J. Veeder
- Book ID
- 102571363
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 63 KB
- Volume
- 139
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
โฆ Synopsis
A near-infrared spectrum of Neptune's satellite Nereid was obtained at the Keck Observatory on 1997 May 1. The spectrum shows two absorptions near 1.54 and 2.03 ยตm and is well matched by a synthetic spectrum of an intimate mix of low-temperature, particulate water ice and dark, bluecolored material. Comparisons of Nereid's spectrum with those of other objects such as the Centaurs 1997 CU 26 and 5145 Pholus, and Neptune's largest regular satellite Proteus, admit the possibility that Nereid is a primordial satellite of Neptune (and perhaps its only remaining one) rather than a captured object, but more data are needed to rule out one scenario or the other.
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