Physical studies of asteroids. IX - The light curve of the M asteroid 77 Frigga

Details Physical studies of asteroids. IX - The light curve of the M asteroid 77 Frigga Physical studies of asteroids. IX - The light curve of the M asteroid 77 Frigga

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982m%26p....27..107l&link_type=abstract

Moon and the Planets, vol. 27, Aug. 1982, p. 107-110.

Physics

6

Asteroids, Electrophotometry, Light Curve, Ubv Spectra, Orbital Elements, Spectrum Analysis, Two Body Problem

Scientific paper

From eight nights of photoelectric UBV observations of the 77 Frigga asteroid during the 1982 opposition, at phase angles smaller than 2.8 deg, a synodic period of 0.3755 + or - 0.0006 days is derived. The light curve appears to be symmetric, with two maxima per period and an amplitude of 0.19 m. B-V and U-V color indices are 0.738 + or 0.003 and 0.2 + or - 0.002 m, respectively, and the primary maximum corresponds to 8.58 m.

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