Other
Scientific paper
Mar 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994lpi....25.1419t&link_type=abstract
In Lunar and Planetary Inst., The Twenty-Fifth Lunar and Planetary Science Conference. Part 3: P-Z p 1419-1420 (SEE N94-35448 11
Other
Mathematical Models, Planetary Surfaces, Planetary Temperature, Pluto (Planet), Scattering, Solid Nitrogen, Spectrum Analysis, Surface Temperature, Absorptivity, Scattering Coefficients
Scientific paper
With Hapke scattering theory and absorption coefficients derived from our laboratory measurements of solid N2 we have modeled the spectrum of Triton. By comparing a Hapke scattering model to the measured spectrum from Triton, we determined the temperature of the N2 on the satellite's surface to be 38 (+2, -1) K which is in accord with the measurements of Voyager 2. Applying this technique to Pluto we find that the temperature of N2 on that body is 40 +/- 2 K. Other aspects of this investigation are discussed.
Brown Harvey R.
Cruikshank Dale P.
Owen Tobias C.
Tryka Kimberly A.
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