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Reflectance Spectra of Titan Tholins at Cryogenic TemperaturesSpectral behavior of room temperature Titan tholin is used to model reflectance spectra of outer solar systems surfaces. We measured the reflectance spectrum of Titan tholin, 100 310 K, and will discuss the impact on compositional interpretation. Additional information is contained in the original extended abstract.
Document ID
20020046057
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Roush, T. R. (NASA Ames Research Center Moffett Field, CA United States)
Dalton, J. B. (NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
PROJECT: RTOP 344-30-30-01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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