NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Spectroscopic determination of the phase composition and temperature of nitrogen ice on TritonLaboratory spectra of the first overtone band (2.1480 microns, 4655.4 reciprocal cm) of solid nitrogen show additional structure at 2.1618 microns (4625.8 reciprocal cm) over a limited temperature range. The spectrum of Neptune's satellite Triton shows the nitrogen overtone band as well as the temperature-sensitive component. The temperature dependence of this band may be used in conjunction with ground-based observations of Triton as an independent means of determining the temperature of surface deposits of nitrogen ice. The surface temperature of Triton is found to be 38.0 +2.0 or -1.0 K, in agreement with previous temperature estimates and measurements. There is no spectral evidence for the presence of alpha-nitrogen on Triton's surface, indicating that there is less than 10 percent carbon monoxide in solid solution with the nitrogen on the surface.
Document ID
19930070171
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Tryka, Kimberly A.
(California Inst. of Technology Pasadena, United States)
Brown, Robert H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Anicich, Vincent
(JPL Pasadena, CA, United States)
Cruikshank, Dale P.
(NASA Ames Research Center Moffett Field, CA, United States)
Owen, Tobias C.
(Hawaii Univ. Honolulu, United States)
Date Acquired
August 16, 2013
Publication Date
August 6, 1993
Publication Information
Publication: Science
Volume: 261
Issue: 5122
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
93A54168
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available