Search Results
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data set:
GASKELL PHOEBE SHAPE MODEL V1.0
Phoebe shape model from Cassini ISSNA and ISSWA images, by R. Gaskell, version of July 7, 2010.
CASSINI-HUYGENS - CO-SA-ISSNA-5-PHOEBESHAPE-V1.0 - starting 2004-06-11T00:00:00Z -
data set:
GASKELL MIMAS SHAPE MODEL V1.0
Mimas shape model from Cassini ISSNA and Voyager 1 ISSN images, by R. Gaskell, version of July 14, 2010.
CASSINI-HUYGENSVOYAGER - CO-SA-ISSNA-5-MIMASSHAPE-V1.0 - starting 1980-11-12T00:00:00Z -
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. -
instrument host:
Cassini Orbiter
Information about the Cassini Orbiter instrument host -
collection:
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 -
collection:
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 -
bundle:
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. -
bundle:
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. -
bundle:
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 -
collection:
Raw Data Collection for the Cassini ISS Observations from the Cruise to Saturn
This is the collection of raw ISS images and associated metadata from the Cassini cruise to Saturn. -
collection:
Raw Data Collection for the Cassini ISS Observations from the Saturn Tour
This is the collection of raw ISS images and associated metadata from the Cassini tour of the Saturn system. -
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.
Data Sets and Information