2 Pallas pole revisited

Details 2 Pallas pole revisited 2 Pallas pole revisited

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983m%26p....28...17b&link_type=abstract

Moon and the Planets (ISSN 0165-0807), vol. 28, Feb. 1983, p. 17-21. Research supported by the Consiglio Nazionale delle Ricerch

Astronomy and Astrophysics

Astronomy

8

Asteroids, Astronomical Photometry, Electrophotometry, Light Curve, Axes Of Rotation, Data Reduction, Periodic Variations, Rotating Bodies

Scientific paper

The observations are made with the 40-cm refractor of the Terramo Astronomical Observatory (Italy). Also used are an analog photometer, a photomultiplier, and filters for the V and B light. The observations are analyzed on the basis of the period arrived at by Schroll et al. (1976) from observations made in 1968, 1970, and 1973. The 1974 light curves are arranged in phase using Schroll's period, and good agreement is found between the morphology of the general light curve (with two maxima and two minima usually present) and the actual light curves. Good agreement is also found with the values established by Schroll et al. for both coordinates of the pole and for the synodic period.

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