Photometric properties of the minor planets: Observations of (1) Ceres in 1972, 1977, 1982, 1984 and 1985

Details Photometric properties of the minor planets: Observations of (1) Ceres in 1972, 1977, 1982, 1984 and 1985 Photometric properties of the minor planets: Observations of (1) Ceres in 1972, 1977, 1982, 1984 and 1985

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jbaa...98..351h&link_type=abstract

Journal of the British Astronomical Association, vol.98, no.7, p.351-354

Astronomy and Astrophysics

Astronomy

2

Photometry, Asteroids

Scientific paper

From visual observations made between 1971 and 1986 the linear portion of the phase curve for (1) Ceres is described by the relationship V (1, a)=3.64 (+/- 0.23) + 0.037 (+/- 0.010)a for phase angles, a between 7 degrees and 54 degrees. The amplitude of variation derived photometrically was 0.04 +/- 0.005 magnitudes. The B - V index was 0.72 +/- 0.015 magnitudes.

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