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SHAPE AND ROTATION OF (8567) 1996 HW1
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.
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연관 데이터
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.
PLATE SHAPE MODEL OF ASTEROID STEINS V1.0
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Shape model of asteroid 2867 Steins, as derived from the Rosetta images obtained around the time of closest approach.
Visual Imaging and Photometry of (29981) 1999 TD10 V1.0
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The outer solar system object (29981) 1999 TD10 was observed in the R band in September 2001, and in B, V, R, and I in October 2002. We derive B-V=0.80+/-0.05mag, V-R=0.48+/-0.05mag, and R-I=0.44+/-0.05mag. Combining our data with the data from Rousselot et. al. 2003, we derive a synodic period of 15.382+/-0.001hr in agreement with the period from Rousselot et. al. 2003. Our observations show no evidence of a coma.
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.
TRANS-NEPTUNIAN OBJECT LIGHTCURVES
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This data set includes a collection of published lightcurves of trans-Neptunian objects published through December 2002. The collection includes lightcurves of 18 TNOs.
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).
ASTEROID LIGHTCURVE DERIVED DATA
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This is a compilation of published rotational parameters derived from lightcurve data for asteroids, based on the Warner et al. (2009) Asteroid Lightcurve Database. This is the version as of February 3, 2017. In addition to reported rotational parameters by individual papers, there is a summary file with the values adopted by Harris, Warner, and Pravec as the most likely correct values for each asteroid. The data set also contains files listing known binary asteroids, asteroid spin axes, and 'tumbling' asteroids.
FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA V1.0
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The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained and used in Sherry Fieber-Beyer's Ph.D. dissertation at the University of North Dakota. The research focused on asteroids in a zone centered on the 3:1 resonance. These spectra were used to mineralogically characterize asteroids in this zone in an attempt to identify their meteorite analogs.
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