Photometric Observations of Minor Planets at ESO - 1976-1979

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The study of the light variation of minor planets allows an estimate of their form and rotation (direction ofaxis and period). If it is furthermore possible to obtain a measure of their apparent magnitude over as long a time interval as possible, then the knowledge of the albedo and orbit gives the absolute magnitude and dimension. A table exists that connects the diameter and the magnitude/albedo; it has been compiled by the method of least squares applied to asteroids for which the diameters have been determined by other methods.

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