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STOOKE SMALL BODY SHAPE MODELS V2.0
This data set contains Philip Stooke shape models for 243 Ida, 253 Mathilde, 951 Gaspra, comet Halley, J5 Amalthea, J14 Thebe, N7 Larissa, N8 Proteus, S10 Janus, S11 Epimetheus, S16 Prometheus, and S17 Pandora, based on optical data from the NEAR, Galileo, Giotto, Vega 1, Vega 2, and Voyager missions.
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STOOKE SMALL BODIES MAPS V1.0
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These maps of small solar system bodies have been prepared by Philip Stooke of the University of Western Ontario. This data set includes 221 map sheets of five asteroids, five planetary satellites, and one comet, all prepared from spacecraft images.
STOOKE SMALL BODIES MAPS V3.0
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These maps of small solar system bodies have been prepared by Philip Stooke of the University of Western Ontario. This data set includes 270 map sheets of six asteroids, five planetary satellites, and three comets, all prepared from spacecraft images. This data set was updated in 2015 with the addition of 44 new map sheets.
RIVKIN THREE MICRON ASTEROID DATA V3.0
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This data set is a collection of 3-micron spectra of 33 asteroids and Phobos and Deimos obtained by Andy Rivkin and collaborators. Nearly all these data have been published.
ASTEROID (101955) BENNU SHAPE MODEL V1.0
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We present the three-dimensional shape of near-Earth asteroid (101955) Bennu (provisional designation 1999 RQ36) based on radar images and optical lightcurves (Nolan et al., 2013). Bennu was observed both in 1999 at its discovery apparition, and in 2005 using the 12.6-cm radar at the Arecibo Observatory and the 3.5-cm radar at the Goldstone tracking station. Data obtained in both apparitions were used to construct a shape model of this object. Observations were also obtained at many other wavelengths to characterize this object, some of which were used to further constrain the shape modeling (Clark et al., 2011; Hergenrother et al., 2013; Krugly et al., 1999).
NASA 3D Models: Ares 1
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Polygons: 3872 Vertices: 2074
NASA 3D Models: Voyager Probe
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Polygons: 99526 Vertices: 50502
SHAPE AND ROTATION OF (8567) 1996 HW1 V1.0
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We present the three-dimensional shape and rotation state of near-Earth asteroid (8567) 1996 HW1 based on radar images and optical lightcurves (Magri et al., 2011). 1996 HW1 was observed in 2008 using the 12.6-cm radar at Arecibo Observatory. Optical lightcurves were obtained at several observatories and used to further constrain the shape modeling.
LEBOFSKY ET AL. 3-MICRON ASTEROID DATA V1.2
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3-micron spectrophotometric data on asteroids collected from several papers by Lebofsky, Jones, and Feierberg and their collaborators, published 1980-1990.
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