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Dataset results
204 results for “shape model”
GASKELL TETHYS SHAPE MODEL V1.0
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided.
GASKELL PHOEBE SHAPE MODEL V2.0
The shape model of Phoebe derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on August 4, 2012. Vertex-facet versions of the models are also provided.
SMALL BODY SHAPE MODELS V2.1
Optical shape models of 10 planetary moons and asteroids, derived from spacecraft imaging by Philip Stooke.
PLATE SHAPE MODEL OF ASTEROID STEINS V1.0
Shape model of asteroid 2867 Steins, as derived from the Rosetta images obtained around the time of closest approach.
GASKELL MIMAS SHAPE MODEL
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided.
SMALL BODY RADAR SHAPE MODELS V2.0
This data set contains radar-based shape models for small solar system bodies, prepared by various authors.
STOOKE SMALL BODY SHAPE MODELS V1.0
Optical shape models of 10 planetary moons and asteroids, derived from spacecraft imaging by Philip Stooke.
SMALL BODY SHAPE MODELS V2.0
Optical shape models of 9 planetary moons and asteroids, derived from spacecraft imaging by P. Thomas
GASKELL ITOKAWA SHAPE MODEL V1.0
The shape model of 25143 Itokawa derived by Robert Gaskell from Hayabusa AMICA images. The model is provided in the implicitly connected quadrilateral (ICQ) format in four levels of resolution. This version of the model was prepared on August 29, 2007. Vertex-facet versions of the models are also provided.
SHAPE MODEL OF ASTEROID (153591) 2001 SN263 V1.0
We present the three-dimensional shapes and rotation states of the three components of near-Earth asteroid (153591) 2001 SN263 based on radar images and optical lightcurves (Becker et al., 2015. 2001 SN263 was observed in 2003 using the 12.6-cm radar at Arecibo Observatory. Optical lightcurves were obtained at several observatories and used to further constrain the shape modeling.
Gaskell Phobos Shape Model V1.0
The shape model of Phobos derived by Robert Gaskell from Viking Orbiter 1 and Phobos 2 images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on March 11, 2006. Vertex-facet versions of the models are also provided.
Small Bodies Radar Shape Models V1.0
This data set contains radar-based shape models for small solar system bodies, prepared by various authors.
ASTEROID (101955) BENNU SHAPE MODEL V1.0
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).
PLATE SHAPE MODEL OF COMET 103P/HARTLEY 2 V1.0
Shape model of comet 103P/Hartley 2, as derived from the Deep Impact spacecraft images obtained around the time of closest approach to the comet during the EPOXI mission. Includes maps of the surface features on the nucleus.
GASKELL DIONE SHAPE MODEL
The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012. Vertex-facet versions of the models are also provided.
DAWN CERES SPC SHAPE MODEL V1.0
The shape model of 1 Ceres derived from Dawn Framing Camera images using the Stereo-photoclinometry method. The model is provided in the implicitly connected quadrilateral (ICQ). This version of the model was prepared on October 19, 2018.
SMALL BODY SHAPE MODELS V1.0
This data set contains the Peter Thomas shape models for small solar system bodies, as well as image mosaics constructed from these models. The current version of the data set contains the following: 243 Ida, 951 Gaspra, M1 Phobos, M2 Deimos, S7 Hyperion, S10 Janus, S11 Epimetheus.
Gaskell Eros Shape Model V1.0
The shape model of 433 Eros derived by Robert Gaskell from NEAR MSI images. The model is provided in the implicitly connected quadrilateral (ICQ) format in four levels of resolution. This version of the model was prepared on Feb. 23, 2008. Vertex-facet versions of the models are also provided.
GASKELL MIMAS SHAPE MODEL V1.0
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 14, 2010. Vertex-facet versions of the models are also provided.
GASKELL MIMAS SHAPE MODEL V2.0
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided.
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Allen Brain Atlas
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International Brain Laboratory public data
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OpenNeuro
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