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- W2118383738 abstract "This paper presents results of modelling light vari- ations of a freely precessing asteroid, assuming its ellipsoidal shape and a geometric light scattering law. The method is based on numerical integration of Euler equations, combined with the explicit expression of an asteroid's brightness as a function of Euler angles. Modelling is applied to simulate the lightcurve of 4179 Toutatis according to its triaxial ellipsoid shape and spin state given by Hudson & Ostro (1995). A good agreement is ob- tained between the frequencies of the simulated and observed lightcurves. The results explain some apparent discrepancies between the periods obtained from photometric and radar ob- servations." @default.
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- W2118383738 date "1999-05-01" @default.
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- W2118383738 title "Relation between rotation and lightcurve of 4179 Toutatis" @default.
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