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Watkins 2018 Lunar Boulder Data
The Watkins 2018 Lunar Boulder PDS4 bundle -
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Clementine Imaging Bundle
This bundle contains observational products from and documentation on the Deep Space Program Science Experiment's Clementine-1 orbiter ("Clementine"). This bundle includes both 'raw' experiment data record (EDR) data and gridded, map-projected mosaic products. This bundle is a translation and modernization of the five PDS3 data sets originally collected in the "Mission to the Moon" archive (MttMA) Volume Series and currently held by the PDS Imaging Node (IMG): * CLEM1-L/E/Y-A/B/U/H/L/N-2-EDR-V1.0 (raw / EDR data; the long series of letters designates the mission phases and instruments included in the archive) * CLEM1-L-U-5-DIM-BASEMAP-V1.0 (single-band 'basemap' mosaic used as a geometric reference for subsequent mosaic products, based on images taken using the Clementine Ultraviolet/Visible Camera (UVVIS)'s 750-nm filter) * CLEM1-L-U-5-DIM-UVVIS-V1.0 (multispectral mosaic from UVVIS) * CLEM1-L-N-5-DIM-NIR-V1.0 (multispectral mosaic from the Clementine Near-Infrared Camera (NIR)) * CLEM1-L-H-5-DIM-MOSAIC-V1.0 (single-band 'strip' mosaic generated from images taken using the Clementine High-Resolution Camera (HIRES)'s 750-nm filter) -
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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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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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Clementine LWIR Derived Brightness Temperature Bundle
Images of lunar surface brightness temperature derived from Clementine Long-Wavelength Infrared (LWIR) images -
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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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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.
Data Sets and Information