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Shapes and scattering properties of large irregular bodies from photometric data

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Abstract

The macroscopic shapes, rotational states, and scattering parameters of atmosphereless bodies can be deduced from photometric measurements of total brightnesses in different viewing/illumination geometries. The problem is solved with nonlinear optimization techniques; the use of positive definite quantities effectively removes the apparent ill-posedness of the problem. Since the parameters of scattering laws such as the Hapke model cannot be unambiguously determined from photometric data only, we propose a simple empirical scattering model for the purpose. Our methods can obtain convex hull-like shapes even for strongly nonconvex objects; a conception of the major concavities can also be formed.

©2001 Optical Society of America

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Supplementary Material (2)

Media 1: MOV (669 KB)     
Media 2: MOV (677 KB)     

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Figures (2)

Fig. 1.
Fig. 1. The shape model and a lightcurve of asteroid 6489 Golevka at two observing geometries [two movies (690 kB, 690 kB)].
Fig. 2.
Fig. 2. The phase function f(α) for asteroid 433 Eros.

Equations (10)

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d L = S ( μ , μ 0 ) ϖ d σ ,
L = A g ,
χ 2 = L A g 2
G ( ϑ , ψ ) = exp ( lm a lm Y l m ( ϑ , ψ ) ) ,
L ( E , E 0 ) = A + S G ( ϑ , ψ ) d σ ,
g j = G ( ϑ j , ψ j ) Δ σ j ,
χ rel 2 = i L ( i ) L - ( i ) A ( i ) g < A ( i ) g > 2 ,
S ( μ , μ 0 , α ) = f ( α ) [ S LS ( μ , μ 0 ) + c S L ( μ , μ 0 ) ]
= f ( α ) μ μ 0 ( 1 μ + μ 0 + c ) ,
f ( α ) = A 0 exp ( α D ) + k α + 1 ,
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