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Data Sets and Information
• bundle: Visual Imaging and Photometry of (29981) 1999 TD10 V2.0
  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.
• bundle: WISNIEWSKI ASTEROID ABSOLUTE MAGNITUDES
  Photometric observations of 125 asteroids, including absolute magnitudes, reported in Wisniewski et al. 1997.
• bundle: Zappala et al. (1995) Asteroid Dynamical Families V1.0
  Dynamical family classification of asteroids by Zappala et al., based on the hierarchical clustering method
• bundle: SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC
  These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B].
• bundle: SPECTROSCOPY AND PHOTOMETRY OF JUPITER TROJANS
  This data set contains the results of the visible spectroscopic and photometric survey of Jupiter Trojans reported in Fornasier et al. 2004 and Fornasier et al. 2007. The survey was carried out in the years 2002-2005 at the 3.5 m New Technology Telescope of the European Southern Observatory at La Silla, Chile. Included are visible spectroscopy and BVRI photometry of 73 Jupiter Trojans.
• bundle: Gartrelle et al. IRTF Asteroid Spectra V1.0
  This data set is comprised of the VNIR (0.69-2.5 micron) spectra of twenty-five D-type asteroids from varying Solar System locations. The spectra were obtained from NASA/IRTF on Mauna Kea between 2016-2019 using the SpeX instrument in Low-Resolution Prism mode and the 0.8 x 15" slit. Guiding was performed using spillover light from the slit (GuideDog) for targets with apparent magnitude > 15.5. For targets fainter than magnitude 15.5, guiding was accomplished using the MORIS CCD imager.
• bundle: Asteroid (101955) Bennu Radar Shape Model V1.1
  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).
• bundle: Asteroid Lightcurve Database (LCDB) V4.0
  The asteroid lightcurve database (LCDB) is one of the more widely-used research tools for those doing research that compares and contrasts physical characteristics of asteroid spin axis rates, sizes, pole orientations, and/or taxonomic class - among others. The v4.0 release includes lightcurve photometry results for 34967 targets. Each object has one to several dozen detail records that contain results obtained by reviewing the literature.
• bundle: OPTICAL CONSTANTS AND LAB SPECTRA OF WATER ICE
  Transmission spectra of amorphous and crystalline H2O-ice at temperatures from 20-150 K for a wavelength range from 1.11 to 2.63 microns. These spectra have not been continuum-corrected or had the infrared interference fringes removed. Optical constants (n and k values) were derived from these laboratory spectra and are included in the data set.
• bundle: REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS
  This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 27 asteroids, 5 Mars-crossing and 22 near-Earth asteroids, observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2008.
• bundle: REDDY VESTA ROTATIONALLY RESOLVED NEAR-INFRARED SPECTRA
  This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of main belt asteroid (4) Vesta observed with the SpeX instrument on NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i, and reported in Reddy et al. (2011). This data set archives reduced, calibrated spectra that were obtained as part of ground-based characterization of Vesta prior to the arrival of Dawn spacecraft. They have been used for detailed rotationally-resolved mineralogical/compositional analysis.
• bundle: ASTEROID ABSOLUTE MAGNITUDES
  Absolute magnitudes and slopes, mostly IAU-adopted with exceptions noted, for all asteroids numbered as of the 2008 April 20 batch of Minor Planet Circulars.
• bundle: ASTEROID ALBEDOS
  This data set comprises a compilation of asteroid albedos for the convenience of the user. Most but not all of the albedos compiled here also appear in other PDS data sets.
• bundle: SDSS MOVING OBJECT CATALOG
  The Sloan Digital Sky Survey (SDSS) Moving Object Catalog 4th release lists astrometric and photometric data for moving objects detected in the SDSS. The catalog includes various identification parameters, SDSS astrometric measurements (five SDSS magnitudes and their errors), and orbital elements for previously cataloged asteroids. The data set also includes a list of the runs from which data are included, and filter response curves.
• bundle: 2MASS ASTEROID AND COMET SURVEY
  This data set includes J, H, and Ks magnitudes from the Two Micron All-Sky Survey (2MASS) for sources which were positionally associated with asteroids, comets, planets, and planetary satellites. This version includes the 2MASS Extended Mission.
• bundle: Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0
  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 by Sherry Fieber-Beyer.
• bundle: Groundbased Observations at McDonald Observatory
  This bundle collects data taken at McDonald Observatory.
• bundle: POLARIMETRY OF TRANSNEPTUNIAN OBJECTS AND CENTAURS
  The bundle contains a summary of polarimetric observations of Transneptunian objects (including Pluto-Charon system) and Centaurs published by March 19, 2013.
• bundle: Asteroid Polarimetric Database V2.0
  The Asteroid Polarimetric Database (APD) is a collection of asteroid polarimetry results compiled by D.F. Lupishko of Karazin Kharkiv National University, Ukraine. It is intended to include most asteroid polarimetry available through November 15, 2021.
• bundle: TNO AND CENTAUR COLORS
  This data set is intended to include published broadband colors of centaurs and Transneptunian Objects (TNOs) published through March 2014. It includes some comets with Centaur orbits. It supersedes all versions of the TNO colors data set EAR-A-3-RDR-TNO-PHOT.
• bundle: UBV MEAN ASTEROID COLORS
  This data set is a compilation of mean U-B and B-V color indices of asteroids, collected from the published literature and from the unpublished Lowell Observatory UBV Asteroid Survey.
• bundle: Gaffey Meteorite Spectra V1.0
  This data set contains 166 laboratory spectra of 108 meteorite samples, as reported by M. J. Gaffey in Gaffey (1976) [GAFFEY1976]. This in turn was based on his PhD thesis work (Gaffey 1974 [GAFFEY1974]).
• bundle: ASTEROID MASSES
  This collection of asteroid masses and densities was compiled from the published literature by Jim Baer, Steve Chesley, and Dan Britt. Size and shape information are included as well to show the source of the tabulated bulk density. This is the version of the compilation as of April 18, 2012.
• bundle: FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA
  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 and archives reduced, calibrated spectra subsequent 2010. 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.
• bundle: POLARIMETRY OF ASTEROID ITOKAWA
  This data set contains the polarimetry of asteroid 25143 Itokawa published in Cellino et al. (2005). The observations were made from June 26 through July 3, 2004 with the Torino photopolarimeter at the 2.15 m telescope of the El Leoncito Observatory in Argentina. The degree of linear polarization was measured in five filters (Johnson-Cousins UBVRI).
• bundle: ASTEROID RADAR
  This data set is intended to include all published groundbased asteroid radar detections. The file is based on the collection of asteroid radar detections established by Steven J. Ostro and currently maintained by Lance A.M. Benner. The file includes disc-integrated radar properties extracted from the published papers.
• bundle: OLIVINE LABORATORY INFRARED ABSORBANCE SPECTRA
  Laboratory measurements quantifying the effect of Fe substituting for Mg in olivine are necessary to distinguish compositional from temperature, grain size and grain shape effects in observational data. This bundle presents room temperature (18-19 degrees Celsius) diamond anvil cell thin film absorption spectra of a large suite of olivines evenly spaced across Mg and Fe compositions at infrared wavelengths. In each file, the left column is the frequency in wave numbers (units: cm**-1). The right column is the chemical absorbance (common logarithm based).
• bundle: TNO AND CENTAUR DIAMETERS, ALBEDOS, AND DENSITIES V1.0
  This data set is a compilation of published diameters, albedos, and densities for Transneptunian Objects (TNOs) and Centaurs. A total of 194 objects are listed, many with more than one entry. This version covers published values through 31 March 2018.
• bundle: IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS
  This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available.
• bundle: CMOR METEOROID STREAM SURVEY
  A seven-year radar survey of meteor showers has been carried out with the Canadian Meteor Orbit Radar (CMOR) from 2002-2008 (Brown et al. 2008, 2010). This survey resulted in the unambiguous detection and orbital characterization of 109 major and minor meteor showers. This data set includes a list of the detected meteor showers along with their orbital parameters.
• bundle: MOTHE-DINIZ ASTEROID DYNAMICAL FAMILIES
  This bundle contains an updated compilation of asteroid families and clusters, resulting from the application of the Hierarchical Clustering Method (HCM) on a set of around 120,000 asteroids with available proper elements. Whenever available, the classification in the Bus taxonomy is provided for family members, based on spectra from the SMASS, SMASS2 and S3OS2 spectroscopic surveys.
• bundle: VILAS ASTEROID SPECTRA
  This data set contains 81 published spectra of asteroids obtained by Faith Vilas during the years 1982 - 1992.
• bundle: Asteroid Photometric Catalog V1.0
  The Asteroid Photometric Catalog (3rd update), Lagerkvist et al. 1993 [LAGERKVISTETAL1993], is a compilation of all asteroid lightcurve photometry published up to and including the year 1992. The dataset includes the lightcurves in digital form and a table of references to all original publications.
• bundle: Radar shape models of asteroids compiled by Lawrence V1.0
  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
• bundle: Small Planetary Satellite Colors V1.0
  This data set is intended to include published colors of small planetary satellites published up through December 2003. Small planetary satellites are defined as all those except the Moon, the Galilean satellites, Titan, and Triton.
• bundle: FORNASIER SPECTRA OF M ASTEROIDS
  This data set contains reduced composite visual and near-infrared spectra of thirty M-type asteroids, observed over the years 2004-2008 and presented in Fornasier et al. (2010). The spectra were taken with the Dolores and NICS instruments at the Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI instruments at the ESO New Technology Telescope (NTT) in Chile, and with the SPeX instrument at the Infrared Telescope Facility (IRTF) in Hawaii. The individual spectra from the various instruments used to produce the composite spectra are also included.
• bundle: ASTEROID ALBEDOS FROM STELLAR OCCULTATIONS
  This data set contains albedos for 57 asteroids determined from diameters obtained from stellar occultations. These albedos are from Shevchenko and Tedesco (2006).
• bundle: SUB-KILOMETER ASTEROID DIAMETER SURVEY (SKADS)
  The Sub-Kilometer Asteroid Diameter Survey (SKADS) (Gladman et al. 2009) acquired good-quality orbital and absolute magnitude (H) determinations for a sample of small main-belt asteroids in order to study the orbital and size distribution beyond H = 15, down to sub-kilometer sizes (H > 18). Based on six observing nights over an 11-night baseline, SKADS detected, measured photometry for, and linked observations of 1087 asteroids which have one-week time baselines or more. This data set contains the astrometry, photometry, and orbits of the 1087 asteroids detected by SKADS.
• bundle: 24-COLOR ASTEROID SURVEY
  This bundle is comprised of asteroid flux data measured in 26 filters using the McCord dual beam photometer, and covering the range 0.32 - 1.08 microns for 285 numbered asteroids, as published in Chapman & Gaffey (1979b) and McFadden, et al. (1984).
• bundle: SDSS-BASED ASTEROID TAXONOMY
  The Sloan Digital Sky Survey Moving Object Catalog (SDSS-MOC) is a large data set that provides five-filter magnitudes and astrometric information for all moving objects identified in the SDSS images (Izevic et al., 2010). The photometric observations were classified by Carvano et al. (2010) into nine taxonomic classes: Vp, Op, Qp, Sp, Ap, Lp, Dp, Xp and Cp, which are related to the classes and complexes of Bus Taxonomy (Bus & Binzel, 2002b). This data set is contains the taxonomic classification of each SDSS detections and its compilation for each observed asteroid.
• bundle: Comet Data Compilations from Published Sources
  The collections in this archive contain results that have been reported in the literature, or in some cases made available by private communication, for various comet properties. Individual collections focus on one or several closely related properties or targets of high interest.
• bundle: SHAPE MODEL OF ASTEROID (153591) 2001 SN263
  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.
• bundle: LEBOFSKY ET AL. 3-MICRON ASTEROID DATA
  3-micron spectrophotometric data on asteroids collected from several papers by Lebofsky, Jones, and Feierberg and their collaborators, published 1980-1990.
• bundle: BUS-DEMEO ASTEROID TAXONOMY
  The Bus-DeMeo asteroid taxonomy classification system, described in DeMeo et al. (2009), is based on reflectance spectrum characteristics for 371 asteroids measured over the wavelength 0.45 to 2.45 microns. This system of 24 classes is constructed using principal component analysis, following most closely the visible wavelength taxonomy of Bus (1999), which itself builds upon the system of Tholen (1984). Nearly all of the Bus taxonomy classes are preserved, with one new class (Sv) defined. This data set includes a table of classifications in the Bus-DeMeo system for the 371 asteroids upon which the system is based. It also includes mean spectra for each of the classes.
• bundle: PRIMASS-L V1.0
  PRIMASS-L is a spectral library that contains the results of the PRIMitive Asteroids Spectroscopic Survey (PRIMASS). As of June 2021 this library contains spectra of about 642 asteroids from 10 families and two groups that had been sparsely studied before. 85% of our targets did not have published spectra and only 40% had visible photometry. PRIMASS-L contains spectra from a variety of ground-based facilities. This survey is ongoing and is expected to contain about 800 spectra by the end of 2022. Making PRIMASS-L publicly available at the Small Bodies Node of the Planetary Data System enables synergies with other data sets containing physical parameters (e.g. polarimetric properties and geometric albedo) and family affiliation. This will push the characterization of the families and primitive material to a new level and will improve our understanding of the evolution of our Solar System and other planetary systems.
• bundle: BINARY MINOR PLANETS V3.0
  The data set lists orbital and physical properties for well-observed or suspected binary/multiple minor planets including the Pluto system, compiled from the published literature as inspired by Richardson and Walsh (2006) and similar reviews (Merline et al., 2003; Noll, 2006; Pravec et al., 2006; Pravec and Harris, 2007; Descamps and Marchis, 2008; Noll et al., 2008; Walsh, 2009). In total 370 companions in 351 systems are included. Data are presented in three tables: one for orbital and physical properties; one for companion designations, discovery information, and reference codes for data values; and one giving full references for each reference code. This data set is complete for binary/multiple components reported through 31 March 2019.
• bundle: BELSKAYA ASTEROID POLARIMETRY
  This data set contains UBVRI polarimetric measurements of ten main belt asteroids and one potentially hazardous near-Earth asteroid (NEA), from Belskaya et al. (2009) and Belskaya et al. (2009b).
• bundle: ALMA Ceres Imaging and Spectrum V1.0
  This archive package contains the calibrated imaging and spectral data, as well as the integrated photometric (lightcurve) data of Ceres at about 1 mm wavelength obtained from the Atacama Large Millimeter/submillimeter Array (ALMA) in October - November 2015, September 2017, and October 2017. The imaging data were collected with the ALMA 12-meter array in all three epochs with Ceres spatially resolved into about 10, 15, and 15 beams, respectively, and have an average frequency of 265 GHz. Each epoch covers one full rotation of Ceres. The lightcurve data of Ceres were derived from the 12-meter images plus the ALMA Compact Array (ACA) data (effective frequency 259.39 GHz) obtained in the October 2017 epoch. The spectral data cover a frequency range of 256.636 - 266.136 GHz.
• bundle: SEVEN COLOR ASTEROID SURVEY
  The Seven-color Asteroid Survey (SCAS) consists of photometry in seven filters from 0.9 to 2.3 microns, of a total of 126 asteroids of types S, K, and M.
• bundle: ASTEROID TAXONOMY
  This data set is a collection of asteroid taxonomic classifications from various classification methods, collected from the literature.

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