Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987icar...69..571r&link_type=abstract
Icarus (ISSN 0019-1035), vol. 69, March 1987, p. 571-574.
Astronomy and Astrophysics
Astronomy
13
Asteroids, Mineral Deposits, Planetary Surfaces, Spectral Reflectance, Surface Temperature, Temperature Effects, Astronomical Spectroscopy, Galileo Project, Near Infrared Radiation, Spatial Resolution, Visible Spectrum, Asteroids, Temperature, Thermal Properties, Reflectance, Surface, Spectra, Astronomy, Visible Light, Near Infrared, Wavelengths, Laboratory Studies, Mineralogy, Silicate, Distribution, Spectrometry, Technique, Experiments
Scientific paper
The visible and near-IR spectral reflectance of some minerals is a function of temperature. Hence, surface temperature variation must be considered for mineralogical interpretation of spectral reflectance data obtained from a spatially resolved surface which has a temperature distribution. An example is presented to illustrate the errors which can be encountered when interpreting the spectral reflectance of a silicate mineral assemblage, measured at various temperatures that might be expected across an asteroid surface. Independent knowledge of the surface temperature distribution would allow the optimal extraction of mineralogical information in such cases.
Roush Ted L.
Singer Robert B.
No associations
LandOfFree
Possible temperature variation effects on the interpretation of spatially resolved reflectance observations of asteroid surfaces does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Possible temperature variation effects on the interpretation of spatially resolved reflectance observations of asteroid surfaces, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible temperature variation effects on the interpretation of spatially resolved reflectance observations of asteroid surfaces will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1456447