urn:nasa:pds:context:investigation:individual.lunar_simulants_fuv_reflectance_gimar_22 1.0 1.21.0.0 Product_Context 2024-04-23 1.0 Initial version urn:nasa:pds:context:facility:laboratory.swri investigation_to_facility urn:nasa:pds:context:facility:laboratory.utsa_kamc investigation_to_facility urn:nasa:pds:context:instrument:swri.swurc investigation_to_instrument urn:nasa:pds:context:instrument:utsa_kamc.hitachi_sem investigation_to_instrument urn:nasa:pds:context:instrument:utsa_kamc.bruker_eds investigation_to_instrument urn:nasa:pds:lunar_simulants_fuv_reflectance_gimar_22:document:gimar_et_al_2022_preprint investigation_to_document urn:nasa:pds:lunar_simulants_fuv_reflectance_gimar_22:document:gimar_et_al_2022_supplements_preprint investigation_to_document 10.1029/2022JE007508 Gimar, C. J., Raut, U., Poston, M. J., Stevanovic, A., Protopapa, S., Greathouse, T. K., et al. (2022). Far-ultraviolet photometric characteristics of JSC-1A and LMS-1 lunar regolith simulants: Comparative investigations with Apollo 10084. Journal of Geophysical Research: Planets, 127, e2022JE007508. Lunar Simulants JSC-1A and LMS-1 Far-ultraviolet Reflectance Individual Investigation 2017-11-20Z 2021-09-15Z This data bundle contains all of the data presented in the paper "Far-Ultraviolet Photometric Characteristics of JSC-1A and LMS-1 Lunar Regolith Simulants: Comparative Investigations With Apollo 10084" as published in Volume 127, Issue 11 of the Journal of Geophysical Research: Planets. The purpose of this study was to measure the far-ultraviolet (FUV) reflectance properties of the lunar simulants JSC-1A and LMS-1 and compare these properties to those found for the Apollo 11 soil sample 10084 (published previously by U. Raut et al.). Comparing the FUV reflectance of these two simulants and the lunar soil sample provided an opportunity to disentangle the potential contributions of mineralogy and space weathering to lunar soil FUV reflectance. This study's results indicated that titanium-bearing mineral content strongly affects the overall brightness of these soils in the FUV, while space weathering features may correlate to differences in the scattering anisotropy of the soils.