Solar System Research

, Volume 44, Issue 4, pp 267–280

The phase ratios of the color index: Mapping of two regions of the near side of the Moon

  • V. G. Kaydash
  • S. Yu. Gerasimenko
  • Yu. G. Shkuratov
  • N. V. Opanasenko
  • Yu. I. Velikodsky
  • V. V. Korokhin
  • M. V. Kaydash
Article

DOI: 10.1134/S0038094610040015

Cite this article as:
Kaydash, V.G., Gerasimenko, S.Y., Shkuratov, Y.G. et al. Sol Syst Res (2010) 44: 267. doi:10.1134/S0038094610040015

Abstract

From the ground-based colorimetry performed for two surface regions of the near side of the Moon, images of the phase ratio of the color index C(600 nm/470 nm) have been built for the phase angles between 2° and 95°. It has been found that for phase angles smaller than α ∼ 40°–50°, the color index of the highlands grows with the phase quicker than that of the mare regions. For larger phase angles, α > 50°, a reverse situation is observed. The laboratory data on the spectrophotometry of the lunar samples confirm the peculiarities found in the phase dependence of color. The influence of multiple scattering on the phase dependence of the color of the mare and highland regions of the Moon are discussed.

Copyright information

© Pleiades Publishing, Ltd. 2010

Authors and Affiliations

  • V. G. Kaydash
    • 1
  • S. Yu. Gerasimenko
    • 1
  • Yu. G. Shkuratov
    • 1
  • N. V. Opanasenko
    • 1
  • Yu. I. Velikodsky
    • 1
  • V. V. Korokhin
    • 1
  • M. V. Kaydash
    • 2
  1. 1.Institute of AstronomyKharkiv National UniversityKharkivUkraine
  2. 2.Kharkiv National University of EconomicsKharkivUkraine