Dependence of latitude brightness distribution over the Lunar disk on albedo and relief

Details Dependence of latitude brightness distribution over the Lunar disk on albedo and relief Dependence of latitude brightness distribution over the Lunar disk on albedo and relief

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..181a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 2, p. 181-187

Physics

4

Scientific paper

We present results of brightness distribution measurements of the lunar disk and laboratory samples at different phase angles in blue and red spectral bands. It is shown for the Moon that the brightness drop with photometric latitude is formed mainly by the micro and mesorelief of the lunar surface. A small decrease of this drop with wavelength is due not so much to an albedo variation as to changes in the microrelief dimension range, which affects the reflection of light by the Moon.

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