We report on a newly discovered morphological feature on the lunar surface, here named Ring-Moat Dome Structure (RMDS). These low domes (a few meters to ~20 m height with slopes <5°) are typically surrounded by narrow annular depressions or moats. We mapped about 2,600 RMDSs in the lunar maria with diameters ranging from tens to hundreds of meters. Four candidate hypotheses for their origin involving volcanism are considered. We currently favor a mechanism for the formation of the RMDS related to modification of the initial lava flows through inflated flow squeeze-ups and/or extrusion of magmatic foams below a cooling lava flow surface. These newly discovered features provide new insights into the nature of emplacement of lunar lava flows, ...
Theoretical analyses, together with the observed style of emplacement of lunar mare volcanic deposit...
Volcanism is the most important endogenic geological process of the Moon, which is closely related t...
The Ina irregular mare patch, an ∼2 × 3 km summit depression on an ancient ∼22 km diameter shield vo...
We report on a newly discovered morphological feature on the lunar surface, here named Ring-Moat Dom...
Newly documented Ring Moat Dome Structures (RMDSs), low mounds typically several hundred meters acro...
Ring-moat dome structures (RMDSs) are small circular mounds of diameter typically about 200 m and ∼3...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
The enigmatic Ina feature on the Moon was recently interpreted to represent extrusive basaltic volca...
Volcanic eruptions on the Moon take place in conditions of low gravity and negligible atmospheric pr...
Ina is an enigmatic volcanic feature on the Moon known for its irregularly shaped mounds, the origin...
Wöhler C, Lena R. Lunar intrusive domes: Morphometric analysis and laccolith modelling. ICARUS. 2009...
The lunar shield volcano Cauchy 5, sitting at the low diameter‐height‐volume end of the population, ...
Ina, a distinctive ~2 × 3 km D-shaped depression, is composed of unusual bulbous-shaped mounds surro...
Irregular mare patches (IMPs) were previously proposed as sites of young lunar volcanism and/or endo...
Theoretical analyses, together with the observed style of emplacement of lunar mare volcanic deposit...
Volcanism is the most important endogenic geological process of the Moon, which is closely related t...
The Ina irregular mare patch, an ∼2 × 3 km summit depression on an ancient ∼22 km diameter shield vo...
We report on a newly discovered morphological feature on the lunar surface, here named Ring-Moat Dom...
Newly documented Ring Moat Dome Structures (RMDSs), low mounds typically several hundred meters acro...
Ring-moat dome structures (RMDSs) are small circular mounds of diameter typically about 200 m and ∼3...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
The enigmatic Ina feature on the Moon was recently interpreted to represent extrusive basaltic volca...
Volcanic eruptions on the Moon take place in conditions of low gravity and negligible atmospheric pr...
Ina is an enigmatic volcanic feature on the Moon known for its irregularly shaped mounds, the origin...
Wöhler C, Lena R. Lunar intrusive domes: Morphometric analysis and laccolith modelling. ICARUS. 2009...
The lunar shield volcano Cauchy 5, sitting at the low diameter‐height‐volume end of the population, ...
Ina, a distinctive ~2 × 3 km D-shaped depression, is composed of unusual bulbous-shaped mounds surro...
Irregular mare patches (IMPs) were previously proposed as sites of young lunar volcanism and/or endo...
Theoretical analyses, together with the observed style of emplacement of lunar mare volcanic deposit...
Volcanism is the most important endogenic geological process of the Moon, which is closely related t...
The Ina irregular mare patch, an ∼2 × 3 km summit depression on an ancient ∼22 km diameter shield vo...