Photometry of AMOR Asteroids 1036 Ganymede and 1139 Atami

Details Photometry of AMOR Asteroids 1036 Ganymede and 1139 Atami Photometry of AMOR Asteroids 1036 Ganymede and 1139 Atami

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rpsct...2...13l&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 13 (SEE N89-29354 24-12) Transl. into ENGLISH from Astronomicheskiy Ve

Astronomy and Astrophysics

Astronomy

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

Scientific paper

UBV photometry was used to determine the light curves of the asteroids Ganymede (July to 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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