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 …

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 …

Assessment of mare basalt gas release patterns during individual eruptions provides the
basis for predicting the effect of vesiculation processes on the structure and morphology of …

Lunar mare regolith is traditionally thought to have formed by impact bombardment of newly
emplaced coherent solidified basaltic lava. We use new models for initial emplacement of …

Mare domes, small shield volcanoes typically<∼ 30 km diameter, are part of the spectrum of
lunar volcanic features that characterize extrusive basalt deposits. We used new spacecraft …

Volcanic activity is the main process for heat-material exchange and circulation for
differentiated planets. All terrestrial planets in the Solar System, the Moon, the satellites of …

Abstract Ina, a distinctive~ 2× 3 km D‐shaped depression, is composed of unusual bulbous‐
shaped mounds surrounded by optically immature hummocky/blocky floor units. The crisp …

Ring‐moat dome structures (RMDSs) are small circular mounds of diameter typically about
200 m and∼ 3–4 m in height, surrounded by narrow, shallow moats. They occur in clusters …

Mare Fecunditatis is a~ 310,000 km2 flat basalt plain located in the low-latitude area of the
Moon. Plenty of volcanic features (multiple episodes of mare basalts, sinuous rilles, lava …

Abstract Newly documented Ring Moat Dome Structures (RMDSs), low mounds typically
several hundred meters across with a median height of~ 3.5 m and surrounded by moats …