Water group exospheres and surface interactions on the Moon, Mercury, and Ceres

N Schörghofer, M Benna, AA Berezhnoy… - Space Science …, 2021 - Springer
Water ice, abundant in the outer solar system, is volatile in the inner solar system. On the
largest airless bodies of the inner solar system (Mercury, the Moon, Ceres), water can be an …

[HTML][HTML] Atmosphere-aware photoclinometry for pixel-wise 3D topographic mapping of Mars

WC Liu, B Wu - ISPRS Journal of Photogrammetry and Remote …, 2023 - Elsevier
High-resolution topographic mapping is essential for scientific investigations and
operational exploration of planets, such as Mars. Photoclinometry, which uses light scattered …

Near-UV and near-IR reflectance studies of lunar swirls: Implications for nanosize iron content and the nature of anomalous space weathering

DT Blewett, BW Denevi, JTS Cahill, RL Klima - Icarus, 2021 - Elsevier
We performed an analysis of spacecraft multispectral images for lunar swirls in order to gain
an improved understanding of optical space weathering on the Moon and its causes. LROC …

Comparative photometric analysis of the Reiner Gamma swirl and Chang'e 5 landing site

M Hess, C Wöhler, L Qiao, M Bhatt - Astronomy & Astrophysics, 2023 - aanda.org
Context. Lunar swirls are bright albedo features only found on the Moon that are still not
entirely understood. It is commonly accepted that reduced space weathering plays a role in …

Unique regolith characteristics of the lunar swirl Reiner Gamma as revealed by imaging polarimetry at large phase angles

M Bhatt, C Wöhler, J Rogall, K Aravind… - Astronomy & …, 2023 - aanda.org
Context. Lunar swirls are high-albedo irregular markings that are generally associated with
prominent magnetic anomalies. The formation of swirls is still unknown. Near-infrared …

[HTML][HTML] The Global Distribution of Water and Hydroxyl on the Moon as Seen by the Moon Mineralogy Mapper (M3)

RN Clark, NC Pearson, TB McCord… - The Planetary …, 2024 - iopscience.iop.org
Abstract The Moon Mineralogy Mapper (M 3) on the Chandrayaan-1 spacecraft provided
nearly global 0.5–3 μm imaging-spectroscopy data at 140 m pixel–1 in 85 spectral bands …

Spectrophotometric and Topographic Correlations within the Mare Ingenii Swirl Region: Evidence for a Highly Mobile Lunar Regolith

D Domingue, J Weirich, F Chuang… - The Planetary …, 2023 - iopscience.iop.org
The spectrophotometric properties of two study areas in the Ingenii swirl region show that
the combined effects of multiple processes are required to explain the regolith's …

Impactor material records the ancient lunar magnetic field in antipodal anomalies

S Wakita, BC Johnson, I Garrick-Bethell… - Nature …, 2021 - nature.com
The Moon presently has no dynamo, but magnetic fields have been detected over numerous
portions of its crust. Most of these regions are located antipodal to large basins, leading to …

Topographic correlations within lunar swirls in mare Ingenii

D Domingue, J Weirich, F Chuang… - Geophysical …, 2022 - Wiley Online Library
The Moon's bright albedo markings, known as swirls, are defined by broad, bright, on‐swirl
areas separated by darker off‐swirl lanes. Their formation mechanism has long been …

The Search for Topographic Correlations within the Reiner Gamma Swirl

JR Weirich, DL Domingue, FC Chuang… - The Planetary …, 2023 - iopscience.iop.org
Lunar swirls have been traditionally considered to be unaffected by topographic changes.
Yet, correlations between areas of high albedo and lower elevations are observed in …