데이터셋 상세
미국
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.
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연관 데이터
SHAPE MODEL OF ASTEROID (153591) 2001 SN263 V1.0
공공데이터포털
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.
SHAPE MODEL OF ASTEROID (153591) 2001 SN263
공공데이터포털
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.
SHAPE AND ROTATION OF (8567) 1996 HW1 V1.0
공공데이터포털
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.
SHAPE AND ROTATION OF (8567) 1996 HW1 V1.0
공공데이터포털
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.
SMALL BODY SHAPE MODELS V1.0
공공데이터포털
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.
Radar shape models of asteroids compiled by Lawrence V1.0
공공데이터포털
This data set contains three-dimensional shape models for asteroids observed by ground-based radar facilities. The data set contains shape models for the following asteroids: (2100) Ra-Shalom (4486) Mithra (4660) Nereus (10115) 1992 SK (29075) 1950 DA (Retrograde and Prograde models) (33342) 1998 WT24 (54509) YORP (66391) 1999 KW4 Alpha (primary) and Beta (secondary) (136617) 1994 CC Alpha (primary) (276049) 2002 CE26 Alpha (primary) (341843) 2008 EV5
ASTEROID (101955) BENNU SHAPE MODEL V1.0
공공데이터포털
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 ASTEROID STEINS V1.0
공공데이터포털
Shape model of asteroid 2867 Steins, as derived from the Rosetta images obtained around the time of closest approach.
PLATE SHAPE MODEL OF ASTEROID STEINS V1.0
공공데이터포털
Shape model of asteroid 2867 Steins, as derived from the Rosetta images obtained around the time of closest approach.
NEAR MSI SHAPE MODEL FOR 433 EROS V1.0
공공데이터포털
This data set contains the Peter Thomas shape model for asteroid 433 Eros, based on optical data from the NEAR MSI instrument.