Resolved Hapke parameter maps of the Moon

H. Sato, Mark Robinson, B. Hapke, B. W. Denevi, A. K. Boyd

Research output: Contribution to journalArticle

49 Citations (Scopus)

Abstract

We derived spatially resolved near-global Hapke photometric parameter maps of the Moon from 21 months of Lunar Reconnaissance Orbiter Camera (LROC) Wide Angle Camera (WAC) multispectral observations using a novel "tile-by-tile method" (1° latitude by 1° longitude bins). The derived six parameters (w,b,c,BS0,hS, andθp) for each tile were used to normalize the observed reflectance (standard angles i = g = 60°, e = 0° instead of the traditional angles i = g = 30°, e = 0°) within each tile, resulting in accurate normalization optimized for the local photometric response. Each pixel in the seven-color near-global mosaic (70°S to 70°N and 0°E to 360°E) was computed by the median of normalized reflectance from large numbers of repeated observations (UV: 50 and visible: 126 on average). The derived mosaic exhibits no significant artifacts with latitude or along the tile boundaries, demonstrating the quality of the normalization procedure. The derived Hapke parameter maps reveal regional photometric response variations across the lunar surface. The b, c (Henyey-Greenstein double-lobed phase function parameters) maps demonstrate decreased backscattering in the maria relative to the highlands (except 321 nm band), probably due to the higher content of both SMFe (submicron iron) and ilmenite in the interiors of back scattering agglutinates in the maria. The hS (angular width of shadow hiding opposition effect) map exhibits relatively lower values in the maria than the highlands and slightly higher values for immature highland crater ejecta, possibly related to the variation in a grain size distribution of regolith. Key PointsSpatially resolved near-global Hapke parameter maps were derived from LROC WACPhotometric properties of the lunar surface vary with wavelength and compositionHighland is more backscattering relative to maria

Original languageEnglish (US)
Pages (from-to)1775-1805
Number of pages31
JournalJournal of Geophysical Research E: Planets
Volume119
Issue number8
DOIs
StatePublished - 2014

Fingerprint

tiles
maria
Moon
Tile
moon
highlands
Lunar Reconnaissance Orbiter
lunar surface
Cameras
cameras
Backscattering
reflectance
backscattering
ilmenite
regolith
Bins
ejecta
longitude
craters
crater

Keywords

  • LROC
  • Moon
  • photometry
  • surface reflectance

ASJC Scopus subject areas

  • Geochemistry and Petrology
  • Geophysics
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Resolved Hapke parameter maps of the Moon. / Sato, H.; Robinson, Mark; Hapke, B.; Denevi, B. W.; Boyd, A. K.

In: Journal of Geophysical Research E: Planets, Vol. 119, No. 8, 2014, p. 1775-1805.

Research output: Contribution to journalArticle

Sato, H. ; Robinson, Mark ; Hapke, B. ; Denevi, B. W. ; Boyd, A. K. / Resolved Hapke parameter maps of the Moon. In: Journal of Geophysical Research E: Planets. 2014 ; Vol. 119, No. 8. pp. 1775-1805.
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