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Watkins 2018 Lunar Boulder Data
The Watkins 2018 Lunar Boulder PDS4 bundle -
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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. -
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Roberts Eros Ponds Catalog V1.1
This data set contains two tables describing the size and location of ponded deposits on asteroid 433 Eros. Both tables contain the same pond information, but one is presented in the format required for ingestion by a publicly available 3D visualization application, the Small Body Mapping Tool (Ernst et al., 2018; http://sbmt.jhuapl.edu). -
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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]. -
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MER Pancam Photometry Archive Bundle
MER Pancam Photometry Archive Bundle -
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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. -
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MER1 Navcam Science Calibrated Radiance Data Bundle
This bundle contains calibrated radiance data from the Navigation Cameras (Navcam) on Mars Exploration Rover 1 (Opportunity). These data were calibrated by the science team. -
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MER2 Microscopic Imager Science Raw Data Bundle
This bundle contains raw data from the Microscopic Imager (MI) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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Nathair Facula Topography and Photometric Cube Data V1.0
This bundle contains regional topography and photometric data for two locations within Nathair Facula, Mercury. Both locations focus on volcanic vents and pyroclastic deposits near 35.86 Lat 63.93 E Lon. The data was generated using the Gaskell Stereophotoclinometry (SPC) software suite with images from the MESSENGER mission to Mercury. In addition to the topographic heights of the Digital Terrain Model (DTM), photometric data is aligned to and has the same horizontal spacing as the topographic data. For select Mercury Dual Imaging System (MDIS) Narrow Angle Camera (NAC) or Wide Angle Camera (WAC) images, four photometric data products are available; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. One DTM represents heights every 120 m and has a size of 130 by 130 km, while the other represents heights every 60 m and has a size of 80 by 80 km. The two DTMs partially overlap. -
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MER1 Pancam Science Derived IOF Data Bundle
This bundle contains derived IOF data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team. -
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Mars Global Cave Candidate Catalog Archive Bundle
The Mars Cave Database -
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HST UV Slitless Reflectance Spectra of (1) Ceres V1.0
This archive package contains the reflectance spectra of Ceres from 121 nm to 198 nm based on the slitless spectrographic observations using HST/ACS SBC performed on 2007 November 25. Ceres was spatially resolved to about 21 pixels in diameter. The raw spectra were extracted from the raw 2D spectral image corresponding to all pixels within the disk of Ceres, calibrated to intensity unit and then to reflectance unit. The final reflectance spectra of Ceres is the average of all spectra over the whole disk of Ceres. All intermediate data and the final average reflectance spectra are included in the data set. -
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Mars Global Cave Candidate Catalog Archive Bundle
Mars Global Cave Candidate Catalog Archive Bundle -
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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. -
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Mars Target Encyclopedia Database Bundle
Information for how to cite the MTE bundle. -
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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. -
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Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System
This bundle contains the digitized products generated from Dr. Ronald Greeley's 35mm Slide Collection, the Jovian System, housed at the RGCPS, ASU, Tempe, AZ. Included is a User’s Guide for a further description of the products. -
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Small Body Optical Shape Models V1.0
The Small Body Shape Models data set contains the Peter Thomas shape models for small solar system bodies, as well as image mosaics constructed from these models. These shape models are based upon optical data from a variety of spacecraft instruments, including the Galileo SSI, NEAR MSI, Viking orbiter, Voyager 1 & 2, and the Hubble Space Telescope. The data has been published in a variety of publications between 1984 and 1999. -
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MER1 Pancam Derived Color Mosaic Data Bundle
This bundle contains color mosaics from the Panoramic Cameras (Pancam) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team. -
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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. -
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EROS MSI IMAGES WITH GEOMETRY BACKPLANES
This data set contains data products for 93,397 images obtained by the Multi-Spectral Imager (MSI) of the Near Earth Asteroid Rendezvous (NEAR) mission during the orbital phase at asteroid 433 Eros. The data products include geometric and geophysical information for each pixel. The data products are in the form of backplanes, stored in the FITS image format. There is one backplane file for each MSI image. Each of the MSI backplane files is a 16-band image cube. The bands of the cube contain the information detailed below calculated for the center of each pixel: 1: Pixel values (I/F) of the original FITS images delivered to the PDS by the NEAR team [Murchie et al., 2001], linearly resampled to rectify the image by squaring the pixels. The original image size is 537 x 244 pixels and the rectified size is 537 x 412 pixels. 2: x coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 3: y coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 4: z coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 5: latitude (planetocentric, degrees) 6: longitude (degrees east) 7: radial distance (kilometers) from the asteroid center of figure 8: solar incidence angle (degrees) 9: emission angle (degrees) 10: solar phase angle (degrees) 11: horizontal pixel scale (kilometers) 12: vertical pixel scale (kilometers) 13: average surface slope relative to gravity (degrees) 14: average elevation relative to gravity (meters) 15: average gravitational acceleration (meters/[s^2]) 16: average gravitational potential (J/kg) -
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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. -
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MER2 Pancam Derived Color Mosaic Data Bundle
This bundle contains color mosaics from the Panoramic Cameras (Pancam) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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ISS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini ISS images, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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GASKELL PHOEBE SHAPE MODEL
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. -
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MER2 Pancam Science Calibrated Data Bundle
This bundle contains calibrated data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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Clementine LWIR Derived Brightness Temperature Bundle
Images of lunar surface brightness temperature derived from Clementine Long-Wavelength Infrared (LWIR) images -
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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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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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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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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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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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NEAR MSI Deblurred Images
2020 PDART - NEAR MSI updated deblurr algorithm. -
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GASKELL TETHYS SHAPE MODEL
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. -
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MER1 Pancam Science Raw Data Bundle
This bundle contains raw data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team. -
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HST images, albedo maps, and shape of (1) Ceres V1.0
This dataset contains 267 HST ACS/HRC images of asteroid (1) Ceres obtained in 2003/2004 at three wavelengths, 535 nm, 335 nm, and 223 nm. They have been photometrically calibrated to standard reflectance unit I/F. The dataset also includes a shape for Ceres, as well as three surface albedo maps covering the area between +/-50 deg latitude, derived from these images. -
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MER2 Navcam Science Calibrated Radiance Data Bundle
This bundle contains calibrated radiance data from the Navigation Cameras (Navcam) on Mars Exploration Rover 2 (Spirit). These data were calibrated by the science team. -
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DELBO THERMAL INFRARED ASTEROID DIAMETERS AND ALBEDOS
This data set contains radiometric albedos and diameters for Near Earth Asteroids (NEAs) derived by three different thermal models and reported in Delbo (2004) [DELBO2004]. The observed infrared fluxes on which the derivations were based are also included. -
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MER2 Microscopic Imager Science Calibrated Data Bundle
This bundle contains calibrated data from the Microscopic Imager (MI) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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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. -
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MER2 Pancam Science Raw Data Bundle
This bundle contains raw data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team. -
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MER1 Microscopic Imager Science Raw Data Bundle
This bundle contains raw data from the Microscopic Imager (MI) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team. -
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NEAR-INFRARED PHOTOMETRY OF ASTEROIDS FROM DENIS
The DENIS program (Deep European Near-Infrared southern sky Survey) was a ground-based survey of the southern sky with the aim of providing an extensive I,J,Ks photometric catalog of point and extended sources. It was carried out at the 1.0 meter ESO telescope at La Silla, Chile from late 1995 through the end of 1999. This data set contains the DENIS I,J,Ks photometry for 2000 known asteroids identified in the DENIS catalog. -
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Saturn Small Moon Shape Models V1.0
Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models typically have uncertainties well under 0.5 km. They are appropriate for global geometric, geologic, and geophysical studies, and regional slope and topography study. They are useful in studying morphologies of only the relatively largest-sized craters. Studies based on early versions of these shape models are in Thomas et al., 2013 -
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Phoebe SPC Shape Model and Assessment Products V1.0
This bundle contains a shape model for the Saturnian moon Phoebe, along with quality assessment data. The global model is similar to the previously archived "Gaskell Phoebe Shape Model", but is provided in multiple formats. -
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LCROSS Impactor Data Bundle
This bundle contains all data collected from instruments onboard the LCROSS Shepherding Spacecraft during its four month mission. Because the purpose of this mission was to observe the impact of a centaur launch stage in a permanently shadowed region of the moon, the most interesting data generated by LCROSS was received just before and after that impact. The bundle contains both raw, partially processed, and calibrated data products. -
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MER Pancam Science Derived Atmospheric Opacity Data Bundle
This bundle contains atmospheric opacity data from the Panoramic Cameras (Pancam) on both Mars Exploration Rovers. These data were produced by the science team. -
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Mars Global Surveyor Mars Orbiter Wide-Angle Camera Photometrically Controlled Mosaics
This product is a modern reprocessing of MOC-WA red and blue limb-to-limb images with a best-effort attempt to photometrically control the images using a Hapke-Henyey-Greenstein photometric model. The full dataset consists of tens of thousands of images which were processed using the United States Geological Survey's Integrated Software for Imagers and Spectrometers (ISIS). -
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IANNINI ASTEROID FAMILY SPECTRA
Keck/ESI spectra of 11 Iannini asteroid family members were obtained over visual wavelengths. The data have been published in Willman, et al. (2008Icar...195...663W)[WILLMANETAL2008]. The spectra show family likeness and are believed to represent young S class surfaces aged a few million years by space weathering, the dynamically estimated collisional age of the family. -
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MER1 Pancam Science Calibrated Data Bundle
This bundle contains calibrated data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team.
Data Sets and Information
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