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Data Sets and Information
• data set: HST SATURN WFPC2 3 RING PLANE CROSSING V1.0
  HST/WFPC2 images of Saturn from before and during the ring plane crossings of 1995
  COMET SL9/JUPITER COLLISIONHSTSATURN RING PLANE CROSSING 1995 - HST-S-WFPC2-3-RPX-V1.0 - starting 1994-10-01T00:00:00Z
• data set: HST S WFPC2 DERIVED ASTROMETRY 2002 V1.0
  This dataset contains astrometric data for eleven Saturn satellites. The data were obtained using the HST/WFPC2 over the period 1994-2002. The volume contains only derived products.
  HSTSATURN SMALL SATELLITE ASTROMETRY - HST-S-WFPC2-4-ASTROM2002-V1.0 - starting 1994-12-01T00:00:00Z
• data set: HST J WFPC2 SL9 IMPACT V1.0
  Hubble Space Telescope (HST) Wide Field Planetary Camera 2 (WFPC2) images of the P/Shoemaker-Levy 9 impact into Jupiter
  COMET SL9/JUPITER COLLISIONHSTSATURN RING PLANE CROSSING 1995 - HST-J-WFPC2-3-SL9-IMPACT-V1.0 - starting 1994-07-15T11:55:16.441Z
• collection: Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, The Jovian System Bodies and Miscellaneous Objects
  This collection, included in document_jovian_system_and_misc, consists of 245 digitized 35mm slides of Jovian System bodies and miscellaneous objects. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in jovian_system_and_misc_diagram_database.pdf and jovian_system_and_misc_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona.
• collection: 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.
• bundle: 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.
• bundle: 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.
• investigation: HST
  Information about the HST investigation
• investigation: HST
  Information about the HST investigation
• instrument host: HUBBLE SPACE TELESCOPE
  Information about the HUBBLE SPACE TELESCOPE instrument host
• collection: 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.
• bundle: 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.
• bundle: 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.
• collection: 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.
• collection: 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.
• collection: 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.
• collection: Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Io
  This collection, included in document_io, consists of 292 digitized 35mm slides primarily of Io, Galilean Satellite of Jupiter, and other related bodies. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in io_diagram_database.pdf and io_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona.
• collection: 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.