Experience with TV photometry of asteroids - The light curve of the asteroid 1727 Mette

Details Experience with TV photometry of asteroids - The light curve of the asteroid 1727 Mette Experience with TV photometry of asteroids - The light curve of the asteroid 1727 Mette

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26...68p&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 4, p. 68-70.

Astronomy and Astrophysics

Astrophysics

2

Asteroids, Astronomical Photometry, Light Curve, Planetary Rotation, Telescopes

Scientific paper

The digital TV complex of the Crimean Astrophysical Observatory was used for photometric observations of the asteroid 1727 Mette (15 m). Ninety measurements in the V-band were made during the nights of April 18, 19, and 20, 1988 at the 0.5-m telescope. The accuracy of a single measurement was +/- 0.04 m, with a 75-s exposure time. The light curve of 1727 Mette has two maxima, and the period is 2.637 +/- 0.004 hr.

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