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Lightcurves and the axis of rotation of 433 Eros

✍ Scribed by J.L. Dunlap


Publisher
Elsevier Science
Year
1976
Tongue
English
Weight
567 KB
Volume
28
Category
Article
ISSN
0019-1035

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The NEAR spacecraft flew by Asteroid 433 Eros on December 23, 1998, and obtained images with a best angular resolution of about 400 m/pixel. These images were used to derive a shape model (Thomas et al. 2000, Icarus). In addition, images obtained at phase angles of 88 β€’ to 115 β€’ during the flyby wer

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We obtained R-band photometry of 433 Eros at the Table Mountain 0.6-m telescope during its 1998 apparition. Our five nights of photometry yields a rotational period P sid = 5.27048 Β± 0.00064 h and visual geometric albedo for 433 Eros of 0.27 +0.03 -0.06 , high, but within the range of S-type asteroi

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Prior to the Near Earth Asteroid Rendezvous (NEAR) mission, little was known about Eros except for its orbit, spin rate, and pole orientation, which could be determined from ground-based telescope observations. Radar bounce data provided a rough estimate of the shape of Eros. On December 23, 1998, a