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Abstract: Near-infrared Hapke photometric analysis of the Moon’s regolith with passive radiometry from the Lunar Orbiter Laser Altimeter (LOLA) (AGU25)

Near-infrared Hapke photometric analysis of the Moon’s regolith with passive radiometry from the Lunar Orbiter Laser Altimeter (LOLA)

Ryan T Walker1, Michael K. Barker1, Erwan Mazarico2, Xiaoli Sun3, Gregory A Neumann1, David E Smith4, Maria T Zuber5 and James W Head III6, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)GSFC, Greenbelt, MD, United States, (4)Massachusetts Institute of Technology, Earth, Atmospheric and Planetary Sciences, Cambridge, MA, United States, (5)Massachusetts Institute of Technology, Earth Atmospheric and Planetary Sciences, Cambridge, United States, (6)Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, United States
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