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- W2014714215 abstract "Models for the shape and global photometric behavior of 243 Ida derived from Galileo images have been used to model the asteroid's telescopic lightcurves. We find excellent agreement between the calculated and observed times of lightcurve extrema, confirming the sidereal rotation period of 4.633632 ± 0.000007 hr determined by Binzelet al. (1993.Icarus105, 310–325.). The shapes and amplitudes of the synthetic and observed lightcurves agree with each other to within ≈0.05 mag, and the average offset in absolute photometry between model and observation is only 0.01 mag. This consistency confirms the accuracy of the shape model derived for Ida by Thomaset al. (1996.Icarus120, 20–32.) and supports the model of the asteroid's photometric behavior developed by Helfensteinet al. (1996.Icarus120, 48–65.)." @default.
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- W2014714215 date "1996-03-01" @default.
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- W2014714215 title "Ida Lightcurves: Consistency with Galileo Shape and Photometric Models" @default.
- W2014714215 doi "https://doi.org/10.1006/icar.1996.0035" @default.
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