Astronomy and Astrophysics, volume 462, L13-16 (2007/1-4)
Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta.
KUEPPERS M., MOTTOLA S., LOWRY S.C., A'HEARN M.F., BARBIERI C., BARUCCI M.A., FORNASIER S., GROUSSIN O., GUTIERREZ P., HVIID S.F., KELLER H.U. and LAMY P.
Abstract (from CDS):
In 2004 asteroid (2867) Steins has been selected as a flyby target for the Rosetta mission. Determination of its spin period and the orientation of its rotation axis are essential for optimization of the flyby planning. Measurement of the rotation period and light curve of asteroid (2867) Steins at a phase angle larger than achievable from ground based observations, providing a high quality data set to contribute to the determination of the orientation of the spin axis and of the pole direction. On March 11, 2006, asteroid (2867) Steins was observed continuously for 24h with the scientific camera system OSIRIS onboard Rosetta. The phase angle was 41.7 degrees, larger than the maximum phase angle of 30 degrees when Steins is observed from Earth. A total of 238 images, covering four rotation periods without interruption, were acquired. The light curve of (2867) Steins is double peaked with an amplitude of ≃0.23mag. The rotation period is 6.052±0.007h. The continuous observations over four rotation periods exclude the possibility of period ambiguities. There is no indication of deviation from a principal axis rotation state. Assuming a slope parameter of G=0.15, the absolute visual magnitude of Steins is 13.05±0.03.
minor planets, asteroids - techniques: photometric
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