urn:nasa:pds:trang2020_moon_space_weathering:data:30ppd_mpfe 1.0 1.14.0.0 Product_Observational 2020-07-21 1.0 Draft by D. Trang 2008-03-14Z 2009-05-09Z Science Derived This map, which is one of three space weathering maps of the Moon, displays the microphase native iron abundance at 30 ppd. The map was derived using the Hapke radiative transfer model. KAGUYA Mission urn:nasa:pds:context:investigation:mission.kaguya data_to_investigation KAGUYA MI KAGUYA Host urn:nasa:pds:context:instrument_host:spacecraft.kaguya is_instrument_host LISM Instrument urn:nasa:pds:context:instrument:kaguya.lism is_instrument Moon Satellite urn:nasa:pds:context:target:satellite.earth.moon data_to_target mpFe display_settings_to_array Sample Left to Right Line Top to Bottom mpFe cartography_parameters_to_image_object 180.0 -180.0 60.0 -60.0 Equirectangular 0.0 0 0.0 Coordinate Pair 1010.7783474716 1010.7783474716 30.0 30.0 -5458203.0763469 1819401.025449 Planetocentric 1737400.0 1737400.0 1737400.0 Positive East urn:nasa:pds:trang2020_moon_space_weathering:document:moon_spaceweathering_map_document data_to_document Description of the space weathering maps and the map derivation. 10.1016/j.icarus.2017.04.026 Trang, D., and P. G. Lucey (2019), Improved Space Weathering Maps of the Lunar Surface Through Radiative Transfer Modeling of Kaguya Multiband Imager Data, Icarus, 321, 307-323. kaguya_mi_derived_30ppd_mpfe.img This product shows the global microphase iron abundance in wt% of the Moon mpFe 0 2 Last Index Fastest IEEE754LSBSingle 1.0 0.0 Line 3600 1 Sample 10800 2