Time-of-day–dependent global distribution of lunar surficial water/hydroxyl

C Wöhler, A Grumpe, AA Berezhnoy… - Science advances, 2017 - science.org
A new set of time-of-day–dependent global maps of the lunar near-infrared water/hydroxyl
(H2O/OH) absorption band strength near 2.8 to 3.0 μm constructed on the basis of Moon …

The new Moon: Major advances in lunar science enabled by compositional remote sensing from recent missions

D Dhingra - Geosciences, 2018 - mdpi.com
Volatile-bearing lunar surface and interior, giant magmatic-intrusion-laden near and far side,
globally distributed layer of purest anorthosite (PAN) and discovery of Mg-Spinel …

Analysis of illumination conditions in the Lunar South Polar Region using multi-temporal high-resolution orbital images

Y Zhang, B Liu, K Di, S Liu, Z Yue, S Han, J Wang… - Remote Sensing, 2023 - mdpi.com
The illumination conditions of the lunar south pole region are complex due to the rugged
terrain and very low solar elevation angles, posing significant challenges to the safety of …

[HTML][HTML] An integrated photogrammetric and photoclinometric approach for illumination-invariant pixel-resolution 3D mapping of the lunar surface

WC Liu, B Wu - ISPRS journal of photogrammetry and remote sensing, 2020 - Elsevier
High-resolution 3D information on lunar and planetary surfaces is crucial for planetary
exploration missions and science. Photogrammetry is a state-of-the-art technology for …

Spectral properties of Martian and other planetary glasses and their detection in remotely sensed data

KM Cannon, JF Mustard, SW Parman… - Journal of …, 2017 - Wiley Online Library
Thirty silicate glasses were synthesized as realistic analogs to those expected to exist on
Mars, the Moon, and Mercury. Samples were measured using visible/near‐infrared and …

Time-of-day-dependent behavior of surficial lunar hydroxyl/water: Observations and modeling

A Grumpe, C Wöhler, AA Berezhnoy, VV Shevchenko - Icarus, 2019 - Elsevier
In this study we determine the depth of the absorption band around 3 µm wavelength, which
indicates the presence of OH/H 2 O in a thin surficial layer of the lunar regolith, for 18 lunar …

Processes governing the VIS/NIR spectral reflectance behavior of lunar swirls

M Hess, C Wöhler, M Bhatt, AA Berezhnoy… - Astronomy & …, 2020 - aanda.org
We investigated six bright swirls associated with magnetic anomalies of variable strength
using Chandrayaan-1 Moon Mineralogy Mapper (M 3) hyperspectral image data. We …

Occurrence and mechanisms of impact melt emplacement at small lunar craters

JD Stopar, BR Hawke, MS Robinson, BW Denevi… - Icarus, 2014 - Elsevier
Using observations from the Lunar Reconnaissance Orbiter Camera (LROC), we assess the
frequency and occurrence of impact melt at simple craters less than 5 km in diameter. Nine …

Temperature regime and water/hydroxyl behavior in the crater Boguslawsky on the Moon

C Wöhler, A Grumpe, AA Berezhnoy, EA Feoktistova… - Icarus, 2017 - Elsevier
In this work we examine the lunar crater Boguslawsky as a typical region of the illuminated
southern lunar highlands with regard to its temperature regime and the behavior of the depth …

Geological mapping of impact melt deposits at lunar complex craters Jackson and Tycho: Morphologic and topographic diversity and relation to the cratering process

D Dhingra, JW Head, CM Pieters - Icarus, 2017 - Elsevier
High resolution geological mapping, aided by imagery and elevation data from the lunar
reconnaissance orbiter (LRO) and Kaguya missions, has revealed the scientifically rich …