author_facet Wilkman, Olli
Muinonen, Karri
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Muinonen, Karri
author Wilkman, Olli
Muinonen, Karri
spellingShingle Wilkman, Olli
Muinonen, Karri
Meteoritics & Planetary Science
Asteroid lightcurve phase shift from rough‐surface shadowing
Space and Planetary Science
Geophysics
author_sort wilkman, olli
spelling Wilkman, Olli Muinonen, Karri 1086-9379 1945-5100 Wiley Space and Planetary Science Geophysics http://dx.doi.org/10.1111/maps.12061 <jats:title>Abstract</jats:title><jats:p>We have simulated asteroid lightcurves for simple shape models using a realistic surface scattering law. The scattering law includes a shadowing function computed with numerical ray‐tracing. We computed lightcurves in a variety of illumination geometries for both the traditional Lommel–Seeliger law and our seminumerical law. We observe a shift in the rotational phase of the lightcurves, which depends on the parameters of the scattering law as well as the illumination geometry and the direction of the spin axis of the asteroid. This phase shift is always zero at opposition, and can be as large as 10° for illumination geometries typical for Main Belt asteroids. The phase shift has implications on the accuracy of other results which are based on asteroid lightcurve analysis, such as spin‐state or shape determination.</jats:p> Asteroid lightcurve phase shift from rough‐surface shadowing Meteoritics & Planetary Science
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title Asteroid lightcurve phase shift from rough‐surface shadowing
title_unstemmed Asteroid lightcurve phase shift from rough‐surface shadowing
title_full Asteroid lightcurve phase shift from rough‐surface shadowing
title_fullStr Asteroid lightcurve phase shift from rough‐surface shadowing
title_full_unstemmed Asteroid lightcurve phase shift from rough‐surface shadowing
title_short Asteroid lightcurve phase shift from rough‐surface shadowing
title_sort asteroid lightcurve phase shift from rough‐surface shadowing
topic Space and Planetary Science
Geophysics
url http://dx.doi.org/10.1111/maps.12061
publishDate 2014
physical 1-7
description <jats:title>Abstract</jats:title><jats:p>We have simulated asteroid lightcurves for simple shape models using a realistic surface scattering law. The scattering law includes a shadowing function computed with numerical ray‐tracing. We computed lightcurves in a variety of illumination geometries for both the traditional Lommel–Seeliger law and our seminumerical law. We observe a shift in the rotational phase of the lightcurves, which depends on the parameters of the scattering law as well as the illumination geometry and the direction of the spin axis of the asteroid. This phase shift is always zero at opposition, and can be as large as 10° for illumination geometries typical for Main Belt asteroids. The phase shift has implications on the accuracy of other results which are based on asteroid lightcurve analysis, such as spin‐state or shape determination.</jats:p>
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description <jats:title>Abstract</jats:title><jats:p>We have simulated asteroid lightcurves for simple shape models using a realistic surface scattering law. The scattering law includes a shadowing function computed with numerical ray‐tracing. We computed lightcurves in a variety of illumination geometries for both the traditional Lommel–Seeliger law and our seminumerical law. We observe a shift in the rotational phase of the lightcurves, which depends on the parameters of the scattering law as well as the illumination geometry and the direction of the spin axis of the asteroid. This phase shift is always zero at opposition, and can be as large as 10° for illumination geometries typical for Main Belt asteroids. The phase shift has implications on the accuracy of other results which are based on asteroid lightcurve analysis, such as spin‐state or shape determination.</jats:p>
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spelling Wilkman, Olli Muinonen, Karri 1086-9379 1945-5100 Wiley Space and Planetary Science Geophysics http://dx.doi.org/10.1111/maps.12061 <jats:title>Abstract</jats:title><jats:p>We have simulated asteroid lightcurves for simple shape models using a realistic surface scattering law. The scattering law includes a shadowing function computed with numerical ray‐tracing. We computed lightcurves in a variety of illumination geometries for both the traditional Lommel–Seeliger law and our seminumerical law. We observe a shift in the rotational phase of the lightcurves, which depends on the parameters of the scattering law as well as the illumination geometry and the direction of the spin axis of the asteroid. This phase shift is always zero at opposition, and can be as large as 10° for illumination geometries typical for Main Belt asteroids. The phase shift has implications on the accuracy of other results which are based on asteroid lightcurve analysis, such as spin‐state or shape determination.</jats:p> Asteroid lightcurve phase shift from rough‐surface shadowing Meteoritics & Planetary Science
spellingShingle Wilkman, Olli, Muinonen, Karri, Meteoritics & Planetary Science, Asteroid lightcurve phase shift from rough‐surface shadowing, Space and Planetary Science, Geophysics
title Asteroid lightcurve phase shift from rough‐surface shadowing
title_full Asteroid lightcurve phase shift from rough‐surface shadowing
title_fullStr Asteroid lightcurve phase shift from rough‐surface shadowing
title_full_unstemmed Asteroid lightcurve phase shift from rough‐surface shadowing
title_short Asteroid lightcurve phase shift from rough‐surface shadowing
title_sort asteroid lightcurve phase shift from rough‐surface shadowing
title_unstemmed Asteroid lightcurve phase shift from rough‐surface shadowing
topic Space and Planetary Science, Geophysics
url http://dx.doi.org/10.1111/maps.12061