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The pole of (51) Nemausa
Authors:L Kahl Kristensen
Abstract:The complex lightcurves make (51) Nemausa a good case for the study of general methods for pole determination. From six lightcurves the pole is determined to 20h24m; +53° (1950); the rotation is retrograde with period 7h.782936 ± 0h.000005. Presence of nongeometric scattering is proved by a significant 0.008 mag amplitude. Formulae and photometric elements are given for predictions of the shapes of lightcurves in future oppositions. The precision of the Fourier coefficients may be reduced below the present ±0.003 mag level by avoiding the systematic errors in the observations due to phase factor variations and discontinuities when changing comparison stars.
Keywords:asteroids: (51) Nemausa
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