Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often
been interpreted as collapsed lava tubes (also known as pyroducts). This hypothesis has …

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 …

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 …

We model the ascent and eruption of lunar mare basalt magmas with new data on crustal
thickness and density (GRAIL), magma properties, and surface topography, morphology and …

Just as the use of new tools revolutionized lunar science in 1610 (Galileo's telescope), 1840
(photography), and 1960s–1970s and 1990s (over 45 robotic and human missions to the …

In less than a decade, the long-held view that the tectonics of the Moon were largely just a
consequence of the evolution of the near side mare basins has been changed dramatically …

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) …

Lunar floor-fractured craters are a class of 170 lunar craters with anomalously shallow,
fractured floors. Two end-member processes have been proposed for the floor formation …

Lunar pits are small (∼ 10–300 m wide) collapse features with vertical walls and sometimes
overhangs. We have identified almost 300 pits, mostly in ponds of cooled impact melt inside …

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 …