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Voyager 1 Jupiter Ephemeris System III Coordinates Bundle
This bundle consists of Voyager 1 Jupiter encounter ephemeris data in System III (1965) left handed coordinates covering the period 1979-03-03 to 1979-03-16. Two versions, both covering the same time period, but containing slightly different data, are provided. One version was generated by the Voyager MAG team from Voyager 1 SEDR, the other by the PDS/PPI node using the VG1_JUP.BSP and PCK00003.TCP SPICE kernels. -
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Hayabusa AMICA Images with Geometry Backplanes V1.0
The Asteroid Multi-band Imaging Camera (AMICA) of the Hayabusa mission to the asteroid 25143 Itokawa obtained 1662 images from May 11, 2003, shortly after launch, until November 19, 2005, after Itokawa encounter. This data set provides derived data products for 1339 of those images that includes geometric information for each pixel. -
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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. -
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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. -
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Lunar Reconnaissance Orbiter LEND Data Bundle
Lunar Reconnaissance Orbiter LEND Data Products -
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JPL Lunar Prospector Gravity Model Bundle
This bundle contains a set of gravity models for the Moon derived by investigators at JPL. -
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Saturn Ring System Solar Occultations Observed by Cassini UVIS
This bundle contains derived time series data products from multiple solar occultations by the rings of Saturn. -
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Magellan Line of Sight Acceleration Profile Bundle
PDS4 Bundle of Magellan Line of Sight Acceleration Profile (LOSAPDR) Data Products -
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NEOWISE Diameters and Albedos V2.0
This PDS data set represents a compilation of published diameters, optical albedos, near-infrared albedos, and beaming parameters for minor planets detected by NEOWISE during the fully cryogenic, 3-band cryo, post-cryo and NEOWISE-Reactivation Years 1 through 3 operations. It contains data covering near-Earth asteroids, Main Belt asteroids, active Main Belt objects, Hildas, Jupiter Trojans, Centaurs, and Jovian and Saturnian irregular satellites. Methodology for physical property determination is described in the referenced articles. -
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Cassini Magnetometer Raw Bundle
This bundle contains Cassini magnetometer raw magnetic field data for the entire mission. The bundle includes magnetic-field data from the Fluxgate Magnetometer and the Vector Helium Magnetomer in Vector mode. Data are received in science and housekeeping rates. Additional collections, such as spacecraft attitude, analog, command validation, configuration image, error counter, user-defined engineering data, browse plots, and calibration, are also included. -
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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. -
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InfraRed Telescope Facility Io Photometry Bundle
IRTF Photometry of Io -
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Uranus System Occultation of Star u14 (Hipparcos 79085) Observed from the ESO 104cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u14 (Hipparcos 79085) by the rings of Uranus. -
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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. -
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Kaguya Gamma-Ray Spectrometer Corrected Spectra Bundle
This archive contains Kaguya Gamma-Ray Spectrometer (KGRS) corrected and calibrated time-series spectra and ephemerides, pointing, and geometry (EPG) data for the nominal and extended observation periods of JAXA's SELENE (Kaguya) mission. The SELENE mission was the Japanese mission to the Moon with a main orbiter “Kaguya” and two daughter relay satellites launched on Sep. 14, 2007. KGRS was mounted on the deck of the main orbiter. It employed a high-purity Ge (HPGe) crystal as a main detector, and surrounding BGO and plastic scintillators as anti-coincidence detectors to reduce backgrounds. The Ge crystal was cooled by a Sterling refrigerator. It made close-proximity observations of the Moon from Dec. 14, 2007 to Dec. 11, 2008 at the high circular orbital altitude of 100 km, and from Feb. 10 to May 28 in 2009 at the low elliptical orbital altitude of ~30 x 50 km. KGRS recorded energy spectra of gamma rays in two gain modes simultaneously; high gain (0.1 to 3 MeV) and low gain (0.1 to 13 MeV), each of which was analyzed by the 13-bit (8192 ch) analog-to-digital converter (ADC). While the former has a higher spectral resolution over the energy range of radioactive elements, the latter has better statistics and covers the whole energy range of major rock-forming elements, including the Fe neutron capture line at 7.6 MeV. The accumulation time of each spectrum was 17 s. Both modes of spectra are included in this archive. The observation epochs of KGRS consists of three regular measurement periods (Period 1 to 3), background measurements, and the annealing of the Ge crystal. The HPGe detector was annealed from 16 to 25, December 2008, which improved energy resolution by a factor of two. Period 1 and 2 lasted two and five months, respectively, with limited spatial or spectral resolutions. Period 3 lasted ~3.5 months (including dead time) with the best spatial and spectral resolutions. In addition, spectra from the background measurement when the satellite was flipped and the detector faced deep space can be analyzed to estimate the background gamma-ray intensity from the satellite due to the exposure to galactic cosmic rays. This archive consists of three spectrum files (each corresponding to one KGRS epoch) and one unified EPG file. The spectrum files contain a time series of corrected and calibrated pulse height spectra acquired by KGRS's HPGe detector in the lunar orbit. In the spectrum files, each row contains the spacecraft clock (sclk) ticks and UTC time corresponding to the end of the accumulation interval (17 s), with the two sets of the 8192-channel HPGe spectra accumulated. In the EPG file, each row starts with sclk recorded at the end of the accumulation interval to match spacecraft positions, pointing, and correction factors with the corrected spectra. Note that the UTC time and ephemeris time included in the EPG file correspond to the midpoint of the accumulation interval. The Kaguya Gamma-Ray Spectrometer Corrected Spectra bundle was created by Naoyuki Yamashita at Planetary Science Institute, AZ, USA, with the permission of JAXA and the KGRS instrument PI Prof. Nobuyuki Hasebe. This work was supported by the NASA under Grant No. NNX16AG54G issued through the Planetary Data Archiving, Restoration, and Tools Program (PDART), Research Opportunities in Space and Earth Sciences (ROSES) 2015. -
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PDS4 System Bundle
This Bundle includes all Collections relevant to the PDS4 System Bundle. -
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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. -
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Uranus System Occultation of Star u1052 (UCAC2 22296665) Observed from the IRTF 320cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u1052 (UCAC2 22296665) by the rings of Uranus. -
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Izenberg PDART 2014 MESSENGER Advanced Products Bundle
MESSENGER Advanced Products (MEAP) by Noam Izenberg, PDART 2014 -
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Apollo 16 ALSEP ARCSAV Lunar Surface Magnetometer Raw Cleaned ASCII Data Bundle
This bundle contains fixed-width ASCII files of daily, raw cleaned measurements acquired by the Lunar Surface Magnetometer (LSM) Experiment at the Apollo 16 landing site for the time span of 02 April through 30 June 1975. These data were extracted from NASA's original Apollo Lunar Surface Experiments Package (ALSEP) archive tapes, also known as ARCSAV tapes. -
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MESSENGER XRS Derived (RDR) Data Bundle
The MESSENGER XRS RDR data consist of maps of the ratio of elements detected by the XRS instrument during orbital operations at Mercury. -
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Uranus System Occultation of Star u9539 (UCAC2 23016546) Observed from the CTIO 400cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u9539 (UCAC2 23016546) by the rings and atmosphere of Uranus. -
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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. -
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Uranus System Occultation of Star u12 (UCAC2 25096598) Observed from the ESO 104cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u12 (UCAC2 25096598) by the rings and atmosphere of Uranus. -
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LCROSS Apache Point Observatory 3.5m Telescope AGILE Data Bundle
This bundle contains data collected from the Apache Point Observatory 3.5m Telescope AGILE instrument during observations of the impact of the LCROSS spacecraft on the moon on October 9, 2009. The bundle contains raw and calibration data products. -
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Uranus System Occultation of Star u0201 (UCAC2 27214859) Observed from the Palomar 508cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u0201 (UCAC2 27214859) by the rings of Uranus. -
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Apollo 17 ALSEP ARCSAV Heat Flow Experiment Raw Cleaned ASCII Data Bundle
This bundle contains fixed-width ASCII files of daily, raw cleaned measurements acquired by the Heat Flow Experiment (HFE) at the Apollo 17 landing site for the time span of 02 April through 30 June 1975. These data were extracted from NASA's original Apollo Lunar Surface Experiments Package (ALSEP) archive tapes, also known as ARCSAV tapes. -
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Uranus System Occultation of Star u23 (UCAC2 22735323) Observed from the CTIO 400cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u23 (UCAC2 22735323) by the rings of Uranus. -
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ISS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini ISS images, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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MESSENGER MDIS Data Archive
Archive of MESSENGER MDIS data, documentation, and anillary files -
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Phoenix ASE Bundle
The original PHX LIDAR dataset was submitted in 2008 -
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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. -
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Magellan ARCDR Bundle
PDS4 Bundle of Magellan Altimetry and Radiometry Composite (ARCDR) Data Products -
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Mars 2020 Navigation Cameras Bundle, stereo products
Stereo data products for the Mars 2020 Perseverance Rover Navigation Cameras. -
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Mars 2020 Navigation Cameras Bundle, mosaic products
Mosaic data products for the Mars 2020 Perseverance Rover Navigation Cameras. -
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Lunar Topography and Photometric Cube Data V1.0
This package contains topography and photometric data generated by the Gaskell Stereophotoclinometry (SPC) software suite. It focuses on six regions on the Moon. These include wrinkle ridges at Dorsa Aldrovandi, two locations of the lunar swirl within Mare Ingenii, Karpinskiy crater, a swirl within Mare Moscoviense, Reiner Gamma, and Tsiolkovskiy crater. We generated regional Digital Terrain Models (DTM), each about 50 to 100 square kilometers, using Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images from both the right and left cameras. Depending on the location, each vertex of the topography represents heights every 5 to 0.7 meters, with an uncertainty of about one to two vertices. The topography data is provided in both cubes readable by the USGS ISIS program, and as a geoTIFF which can be read by programs such as ArcGIS. We generated photometric data (in cube format) that is aligned to, and has the same horizontal spacing as, the topographic cube data. For each LROC image, four cubes were generated; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. Each cube pixel represents the value at each vertex of the DTM. -
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Astro Material Database Archive, chemical analytic data from extraterrestrial materials
This is an archive of laboratory data acquired on astromaterials samples; Archive assembled by S.M. Richard and Peng Ji -
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Mars InSight Lander Document Archive
The Mars InSight Lander document bundle includes a collection of documents for each of the InSight science experiments and a collection of documents pertaining to the mission as a whole. -
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MESSENGER MAG Calibrated Data Bundle
This data set consists of the MESSENGER MAG calibrated observations. The MAG experiment is a miniature three-axis ring-core fluxgate magnetometer with low-noise electronics. There are five MAG data products, which mainly differ in the coordinate system. For each type the data are provided at full resolution, and one or more averaging intervals. -
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Uranus System Occultation of Star u0 (Hipparcos 71567) Observed from the Kuiper Airborne Observatory 91cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u0 (Hipparcos 71567) by the rings and atmosphere of Uranus. -
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MESSENGER EPPS Engineering Raw Data Bundle
This bundle contains the MESSENGER Energetic Particle and Plasma Spectrometer (EPPS) engineering data and the raw data SIS document. These data are associated with the MESSENGER EPPS EPS Raw Data Bundle, and the MESSENGER EPPS FIPS Raw Data Bundle. -
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MER2 Pancam Science Derived IOF Data Bundle
This bundle contains derived IOF data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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Apollo 17 ALSEP Work Tape Lunar Ejecta And Meteorites Experiment Raw Cleaned ASCII Data Bundle
This bundle contains fixed-width ASCII files of raw cleaned measurements acquired by the Lunar Ejecta And Meteorites (LEAM) Experiment at the Apollo 17 landing site for the time span of 01 March through 18 July 1976, which were the last 140 days of LEAM operation. These data were extracted from ALSEP normal-bit-rate Work Tape files. -
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MER MB Relative Iron Abundance Data Bundle
This bundle contains relative iron abundances derived from from the Moessbauer Spectrometer (MB) on both Mars Exploration Rovers (Spirit and Opportunity). -
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MER2 APXS Raw Data Bundle
This bundle contains raw data from the Alpha Particle X-ray Spectrometer on Mars Exploration Rover 2 (Spirit). -
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RELAB Spectral Library Bundle
The RELAB Spectral Library Bundle contains reflectance spectra and ancillary data acquired at the Reflectance Experiment Laboratory (RELAB) at Brown University. -
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Uranus System Occultation of Star u36 (UCAC4 133-156970) Observed from the Maunakea UKIRT 380cm Telescope
This bundle contains calibrated and derived data resulting from the occultation of star u36 (UCAC4 333-124092) by the rings of Uranus. -
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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). -
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Gaskell Eros Shape Model V1.1
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. -
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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.
Data Sets and Information