Photometry of the lunar surface during lunar eclipses

Details Photometry of the lunar surface during lunar eclipses Photometry of the lunar surface during lunar eclipses

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980m%26p....23...99s&link_type=abstract

Moon and the Planets, vol. 23, Aug. 1980, p. 99-107.

Astronomy and Astrophysics

Astronomy

2

Electrophotometry, Lunar Eclipses, Lunar Surface, Brightness, Reflectors, Spectrophotometry

Scientific paper

Photometric observations of the lunar surface during lunar eclipses were performed on four nights between 1972 and 1978 using the 91-cm reflector of the Tokyo Astronomical Observatory. The photometry was performed in B, V, and R and arranged in accordance with the angular distance from the center of the earth's shadow. The results do not show any large systematic differences between the four nights; this means that Danjon's proposition concerning changes of the lunar brightness during eclipses with solar cycles is not confirmed.

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