Add to ORKGTerrestrial planetary bodies are characterized by extensive, largely volcanic deposits covering their surfaces. On Earth large igneous provinces (LIPs) abound, maria cover the nearside of the Moon, and volcanic plains cover large portions of Venus, Mars and Mercury
The spatial distribution of lunar smooth plains is not consistent with experimental simulations of m...
International audiencePartially buried craters on the Moon are those craters whose distal ejecta are...
A model was derived enabling the interpretation of lunar styles of volcanism through the analysis of...
To understand the impact cratering record on Venus, we investigate two distinct resurfacing styles: ...
abstract: Previous workers hypothesized that lunar Localized Pyroclastic Deposits (LPDs) represent p...
abstract: Impact cratering and volcanism are two fundamental processes that alter the surfaces of th...
Abstract. Estimates of lava volumes on planetary surfaces provide important data on the lava floodin...
New measurements of the topography of the Moon from the Lunar Orbiter Laser Altimeter (LOLA)[1] prov...
The consensus regarding interpretation of Magellan radar imagery assigns Venus a young volcanic surf...
Early extrusive volcanism from mantle melting marks the transition from primary to secondary crust f...
Volcanic plains identified on Mercury are morphologically similar to lunar mare plains but lack cons...
One of the most fundamental questions in the geological and thermal evolution of the Moon is the nat...
Although crater modification on the Earth, Moon, and Mars results from surface erosion and crater in...
Terrestrial geologic mapping techniques are regularly used for "photogeologic" mapping of other plan...
The Magellan spacecraft has mapped nearly 99% of the surface of Venus with high resolution synthetic...
The spatial distribution of lunar smooth plains is not consistent with experimental simulations of m...
International audiencePartially buried craters on the Moon are those craters whose distal ejecta are...
A model was derived enabling the interpretation of lunar styles of volcanism through the analysis of...
To understand the impact cratering record on Venus, we investigate two distinct resurfacing styles: ...
abstract: Previous workers hypothesized that lunar Localized Pyroclastic Deposits (LPDs) represent p...
abstract: Impact cratering and volcanism are two fundamental processes that alter the surfaces of th...
Abstract. Estimates of lava volumes on planetary surfaces provide important data on the lava floodin...
New measurements of the topography of the Moon from the Lunar Orbiter Laser Altimeter (LOLA)[1] prov...
The consensus regarding interpretation of Magellan radar imagery assigns Venus a young volcanic surf...
Early extrusive volcanism from mantle melting marks the transition from primary to secondary crust f...
Volcanic plains identified on Mercury are morphologically similar to lunar mare plains but lack cons...
One of the most fundamental questions in the geological and thermal evolution of the Moon is the nat...
Although crater modification on the Earth, Moon, and Mars results from surface erosion and crater in...
Terrestrial geologic mapping techniques are regularly used for "photogeologic" mapping of other plan...
The Magellan spacecraft has mapped nearly 99% of the surface of Venus with high resolution synthetic...
The spatial distribution of lunar smooth plains is not consistent with experimental simulations of m...
International audiencePartially buried craters on the Moon are those craters whose distal ejecta are...
A model was derived enabling the interpretation of lunar styles of volcanism through the analysis of...