Lunar mare basaltic volcanism: Volcanic features and emplacement processes

JW Head, L Wilson, H Hiesinger… - … in Mineralogy and …, 2023 - pubs.geoscienceworld.org
Volcanism is a fundamental process in the geological evolution of the Moon, providing clues
to the composition and structure of the mantle, the location and duration of interior melting …

Return to the Moon: New perspectives on lunar exploration

Y Lin, W Yang, H Zhang, H Hui, S Hu, L **ao, J Liu… - Science Bulletin, 2024 - Elsevier
Lunar exploration is deemed crucial for uncovering the origins of the Earth-Moon system
and is the first step for advancing humanity's exploration of deep space. Over the past …

Generation, ascent and eruption of magma on the Moon: New insights into source depths, magma supply, intrusions and effusive/explosive eruptions (Part 2 …

JW Head, L Wilson - Icarus, 2017 - Elsevier
We utilize a theoretical analysis of the generation, ascent, intrusion and eruption of basaltic
magma on the Moon to develop new insights into magma source depths, supply processes …

Potential melting of extrasolar planets by tidal dissipation

DZ Seligman, AD Feinstein, D Lai… - The Astrophysical …, 2024 - iopscience.iop.org
Tidal heating on Io due to its finite eccentricity was predicted to drive surface volcanic
activity, which was subsequently confirmed by the Voyager spacecraft. Although the volcanic …

Confirmation of sublunarean voids and thin layering in mare deposits

MS Robinson, JW Ashley, AK Boyd, RV Wagner… - Planetary and Space …, 2012 - Elsevier
Typical flow thicknesses of lunar mare basalts were not well constrained in the past,
because as craters and rilles age, downslope movement of loose material tends to mix and …

Distribution, formation mechanisms, and significance of lunar pits

RV Wagner, MS Robinson - Icarus, 2014 - Elsevier
Abstract Lunar Reconnaissance Orbiter Camera images reveal the presence of steep-
walled pits in mare basalt (n= 8), impact melt deposits (n= 221), and highland terrain (n= 2) …

Impacts drive lunar rockfalls over billions of years

VT Bickel, J Aaron, A Manconi, S Loew… - Nature communications, 2020 - nature.com
Past exploration missions have revealed that the lunar topography is eroded through mass
wasting processes such as rockfalls and other types of landslides, similar to Earth. We have …

Lunar science for landed missions workshop findings report

ER Jawin, SN Valencia, RN Watkins… - Earth and Space …, 2019 - Wiley Online Library
Abstract The Lunar Science for Landed Missions workshop was convened at the National
Aeronautics and Space Administration Ames Research Center on 10–12 January, 2018 …

The regolith properties of the Chang'e-5 landing region and the ground drilling experiments using lunar regolith simulants

Y Qian, L **ao, S Yin, M Zhang, S Zhao, Y Pang… - Icarus, 2020 - Elsevier
Abstract The Chang'e-5 (CE-5) mission is China's first lunar sample return mission. The
Rümker region in northern Oceanus Procellarum was selected as the landing area. CE-5 …

Volcanism and deep structures of the Moon

J Zhao, L Qiao, F Zhang, Y Yuan, Q Huang… - Space: Science & …, 2023 - spj.science.org
Volcanism is the most important endogenic geological process of the Moon, which is closely
related to its internal structure and thermal history. Lunar volcanism is one of the most …