1580 Betulia - an unusual asteroid with an extraordinary lightcurve

Details 1580 Betulia - an unusual asteroid with an extraordinary lightcurve 1580 Betulia - an unusual asteroid with an extraordinary lightcurve

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978icar...35..344t&link_type=abstract

Icarus, vol. 35, Sept. 1978, p. 344-359. NASA-supported research.

Astronomy and Astrophysics

Astronomy

12

Asteroids, Astronomical Photometry, Light Curve, Ubv Spectra, Electrophotometry, Graphs (Charts), Phase Shift, Planetary Rotation, Asteroids, Inclination, Perihelion, Carbon, Photometry, Colors, Polarimetry, Albedo, Optical Properties, Mars, Rotation, Wavelengths, Models, Light Curve, Betulia, Amor Asteroids, Comets, Earth-Based Observations, Topography

Scientific paper

Results of UBV photometry and polarimetry of 1580 Betulia during its 1976 apparition are presented. The synodic period of rotation is found to be 6.130 hr. The linear phase coefficient and absolute magnitude of the primary maximum in V are 0.032 mag/deg and 14.88, respectively. No color variations with rotation or solar phase angle were detected, the mean colors being B-V = 0.66 and U-B = 0.24. Betulia's light curve is unique among asteroids studied to date in that it displays three maxima and three minima within one rotational cycle, indicative of a region of greater roughness and/or a dark spot on one of its broad faces. Polarization results indicate a low albedo and a mean diameter of about 7 km, establishing Betulia as the first C-type asteroid to be found among the Mars crossers. A model accounting for most features of Betulia's light curve is given by a prolate spheroid rotating about one of its shorter axes having an axis ratio of 1:1.21 with a major topographic feature on one of its broad faces.

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