Photometry of the AMOR type asteroids 1036 Ganymede and 1139 Atami

Details Photometry of the AMOR type asteroids 1036 Ganymede and 1139 Atami Photometry of the AMOR type asteroids 1036 Ganymede and 1139 Atami

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..167l&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, Apr.-June 1988, p. 167-173. In Russian.

Astronomy and Astrophysics

Astronomy

2

Amor Asteroid, Astronomical Photometry, Ubv Spectra, Amplitudes, Light Curve, Planetary Rotation

Scientific paper

UBV photometry was used to determine the light curves of the asteroids Ganymede (July-November, 1985) and Atami (October, 1986). Their amplitudes amount to 0.40 and greater than 0.18 m, respectively. Ganymede is found to have a period of 10 h 18.25 + or - 0.16 m and a straight direction of rotation. The probable value for the period of Atami is greater than about 20 h.

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