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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: | Jungfrau |
| 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:
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