The rotation period and pole orientation of asteroid 4 Vesta

Details The rotation period and pole orientation of asteroid 4 Vesta The rotation period and pole orientation of asteroid 4 Vesta

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icar...62..298t&link_type=abstract

Icarus (ISSN 0019-1035), vol. 62, May 1985, p. 298-304. NASA-NSF-supported research.

Astronomy and Astrophysics

Astronomy

15

Astrometry, Astronomical Photometry, Planetary Rotation, Vesta Asteroid, Attitude (Inclination), Light Curve, Asteroids, Vesta, Rotation, Period, Astronomy, Observations, Photometry, Lightcurves, Physical Properties, Characteristics

Scientific paper

In 1971 asteroid Vesta was observed in a region of the sky in which it had never been observed before. Its photometric lightcurve had two distinct maxima. Those observations have been the only strong evidence to support a rotation period of about 10 hr 41 min. Lightcurves made in 1982, when Vesta was at the same aspect as 1971, do not show two different maxima. It is concluded that there was a systematic error in the 1971 observations. At this time a definitive statement cannot be made about the true period of Vesta, although the 5 hr 20 min period does appear more plausible. Radar echoes in 1988 and 1992 should resolve the problem. The shorter rotation period was assumed and the photometric astrometry method applied. The sidereal period is 5 hr 20 min 31.68 sec (0.2225889 + or 0.0000002 days), the rotation is prograde, and the coordinates of the north pole are 103 deg longitude and + 43 deg latitude with an uncertainty of about 6 deg.

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