Experience in CCD Spectrocolorimetry of Lunar-Surface Regions

Details Experience in CCD Spectrocolorimetry of Lunar-Surface Regions Experience in CCD Spectrocolorimetry of Lunar-Surface Regions

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sosyr..36..160t&link_type=abstract

Solar System Research, v. 36, Issue 2, p. 160-167 (2002).

Physics

Scientific paper

Panoramic scans of two lunar regions (Aristarchus-Herodotus and Plato craters) were obtained with a CCD camera and spectrograph to determine a range of actual color differences. The color differences expressed in color-excess (CE) units and determined as the intensity ratios for lunar features at 440 and 550 nm are mainly less than 0.1^m. The color-albedo dependence is revealed only in separate clusters and is not the same in different parts of each region under consideration. This special feature of crater Aristarchus is confirmed; that is, in spite of its high albedo, the color in the crater is intermediate within the general range of color differences.

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