{"@type": "dcat:Dataset", "accessLevel": "public", "accrualPeriodicity": "irregular", "bureauCode": ["026:00"], "contactPoint": {"@type": "vcard:Contact", "fn": "Thomas Morgan", "hasEmail": "mailto:thomas.h.morgan@nasa.gov"}, "description": "Digital shape models have been constructed from Cassini Imaging Science Subsystem\n(ISS) data for eleven of the small satellites of Saturn and delivered to the\nPlanetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus,\nPandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models\ntypically have uncertainties well under 0.5 km. They are appropriate for global\ngeometric, geologic, and geophysical studies, and regional slope and topography\nstudy. They are useful in studying morphologies of only the relatively largest-sized\ncraters. Studies based on early versions of these shape models are in Thomas et al.,\n2013", "identifier": "urn:nasa:pds:saturn_satellite_shape_models", "issued": "2021-05-21", "keyword": ["none"], "landingPage": "https://pds.nasa.gov/ds-view/pds/viewBundle.jsp?identifier=urn%3Anasa%3Apds%3Asaturn_satellite_shape_models&version=1.0", "license": "http://www.usa.gov/publicdomain/label/1.0/", "modified": "2025-07-17", "programCode": ["026:005"], "publisher": {"@type": "org:Organization", "name": "National Aeronautics and Space Administration"}, "references": ["https://pds.nasa.gov"], "theme": ["Earth Science"], "title": "Saturn Small Moon Shape Models V1.0"}