Worldwide photometry and lightcurve observations of 1 Ceres during the 1975-1976 apparition

Details Worldwide photometry and lightcurve observations of 1 Ceres during the 1975-1976 apparition Worldwide photometry and lightcurve observations of 1 Ceres during the 1975-1976 apparition

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...54...23t&link_type=abstract

Icarus (ISSN 0019-1035), vol. 54, April 1983, p. 23-29. Research supported by Government of Western Australia, Fonds zur Foerder

Astronomy and Astrophysics

Astronomy

20

Ceres Asteroid, Light Curve, Spectrophotometry, Ubv Spectra, Magnitude, Tables (Data), Asteroids, 1 Ceres, Lightcurves, Photometry, Astronomy, Observations, Apparitions, Periods, Magnitude, Wavelengths, Ultraviolet, Infrared

Scientific paper

Lightcurves and UBV photometry of Ceres from the 1975-1976 apparition are presented. The synodic period is 0.37812 + or 0.00004 day, the mean absolute V magnitude is 3.61 + or 0.03, and the phase coefficient is 0.040 + or - 0.001 mag/deg. The U-B and B-V phase coefficients are +0.0015 + or - 0.0007 and +0.0006 + or - 0.0003 mag/deg, respectively. The colors at zero phase are B-V = +0.70 + or - 0.01 and U-B = +0.41 + or 0.01.

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