Synthetic curves of some observational properties of contact binary asteroids

Details Synthetic curves of some observational properties of contact binary asteroids Synthetic curves of some observational properties of contact binary asteroids

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991an....312..201h&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 312, no. 3, 1991, p. 201-207.

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Asteroids, Planetary Structure, Planetology, Geodesy, Light Curve

Scientific paper

The shape of some asteroids may be deduced by other ground based means than rotation light curves or advanced techniques like speckle imaging or radar observations: the analysis of high precision astrometry and lunar occultation light curves. Calculations of the phenomena among the cosmogonically interesting case of a double asteroid configuration, when the objects are in contact with each other, are presented with special emphasis on the involved shadow phenomena.

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