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HD 102096


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Light curves of asteroid 51 NEMAUSA during its 1989 apparition
Light curves of 51 Nemausa were obtained during 5 nights in 1989. It isfound that the shape of the light curves of the asteroid is stronglydependent on the phase angle. The maximum amplitude increases from 0.11to 13 m as the phase angle increases from 5.4 to 26.5 deg. The meanvalue of the phase coefficient is 0.045 magnitude/deg.

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Observation and Astrometry data

Constellation:Vierge
Right ascension:11h45m01.38s
Declination:-00°31'04.2"
Apparent magnitude:7.311
Distance:128.041 parsecs
Proper motion RA:-30.3
Proper motion Dec:-97.1
B-T magnitude:8.49
V-T magnitude:7.409

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 102096
TYCHO-2 2000TYC 4931-439-1
USNO-A2.0USNO-A2 0825-07545798
HIPHIP 57306

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