Commercial lunar propellant architecture: A collaborative study of lunar propellant production

D Kornuta, A Abbud-Madrid, J Atkinson, J Barr… - Reach, 2019 - Elsevier
Aside 2 from Earth, the inner solar system is like a vast desert where water and other
volatiles are scarce. An old saying is,“In the desert, gold is useless and water is priceless.” …

Exploring the composition of Europa with the upcoming Europa Clipper mission

TM Becker, MY Zolotov, MS Gudipati… - Space Science …, 2024 - Springer
Jupiter's icy moon, Europa, harbors a subsurface liquid water ocean; the prospect of this
ocean being habitable motivates further exploration of the moon with the upcoming NASA …

Direct evidence of surface exposed water ice in the lunar polar regions

S Li, PG Lucey, RE Milliken… - Proceedings of the …, 2018 - National Acad Sciences
Water ice may be allowed to accumulate in permanently shaded regions on airless bodies in
the inner solar system such as Mercury, the Moon, and Ceres [Watson K, et al.(1961) J …

Evidence for exposed water ice in the Moon's south polar regions from Lunar Reconnaissance Orbiter ultraviolet albedo and temperature measurements

PO Hayne, A Hendrix, E Sefton-Nash, MA Siegler… - Icarus, 2015 - Elsevier
We utilize surface temperature measurements and ultraviolet albedo spectra from the Lunar
Reconnaissance Orbiter to test the hypothesis that exposed water frost exists within the …

Water on the surface of the Moon as seen by the Moon Mineralogy Mapper: Distribution, abundance, and origins

S Li, RE Milliken - Science advances, 2017 - science.org
A new thermal correction model and experimentally validated relationships between
absorption strength and water content have been used to construct the first global …

Evidence for surface water ice in the lunar polar regions using reflectance measurements from the Lunar Orbiter Laser Altimeter and temperature measurements from …

EA Fisher, PG Lucey, M Lemelin, BT Greenhagen… - Icarus, 2017 - Elsevier
We find that the reflectance of the lunar surface within 5° of latitude of the South Pole
increases rapidly with decreasing temperature, near∼ 110 K, behavior consistent with the …

Evidence of water on the lunar surface from Chang'E-5 in-situ spectra and returned samples

J Liu, B Liu, X Ren, C Li, R Shu, L Guo, S Yu… - Nature …, 2022 - nature.com
The distribution range, time-varying characteristics, and sources of lunar water are still
controversial. Here we show the Chang'E-5 in-situ spectral observations of lunar water …

Resource potential of lunar permanently shadowed regions

HM Brown, AK Boyd, BW Denevi, MR Henriksen… - Icarus, 2022 - Elsevier
The lunar polar regions contain permanently shadowed regions (PSRs) or local topographic
depressions that never receive direct sunlight. These environments (< 110 K) have the …

Evidence for water ice on the Moon: Results for anomalous polar craters from the LRO Mini‐RF imaging radar

PD Spudis, DBJ Bussey, SM Baloga… - Journal of …, 2013 - Wiley Online Library
The Mini‐RF radar instrument on the Lunar Reconnaissance Orbiter spacecraft mapped
both lunar poles in two different RF wavelengths (complete mapping at 12.6 cm S‐band and …

Seasonal polar temperatures on the Moon

JP Williams, BT Greenhagen, DA Paige… - Journal of …, 2019 - Wiley Online Library
Abstract The Diviner Lunar Radiometer Experiment on the Lunar Reconnaissance Orbiter
has been acquiring visible and infrared radiance measurements of the Moon for nearly 10 …