Add to ORKGLunar sinuous rilles are thought to have formed by thermal erosion, mechanical erosion, construction, or a combination of these processes via emplacement by lava tubes or lava channels. The investigation of Hadley Rille by Apollo 15 provided the first field observations of a rille, but remote sensing observations remain our primary method for studying these features. Terrestrial volcanic features with similar morphologies to lunar rilles can provide insight into their formation on the Moon
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...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
Hadley Rille is directly related to the emplacement of mare basalts in Palus Putredinis. Existing hy...
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...
Lunar sinuous rilles have long been interpreted as features that formed as the result of surficial l...
In order to better understand the processes responsible for the formation of lunar sinuous rilles, a...
We have surveyed lunar sinuous rilles and other volcanic features in an effort to locate intact lava...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
The regional setting, external and internal shape, and materials of Hadley Rille near the Apollo 15 ...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
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...
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...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...
Hadley Rille is directly related to the emplacement of mare basalts in Palus Putredinis. Existing hy...
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...
Lunar sinuous rilles have long been interpreted as features that formed as the result of surficial l...
In order to better understand the processes responsible for the formation of lunar sinuous rilles, a...
We have surveyed lunar sinuous rilles and other volcanic features in an effort to locate intact lava...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
The regional setting, external and internal shape, and materials of Hadley Rille near the Apollo 15 ...
Sinuous collapse chains and skylights in lunar and Martian volcanic regions have often been interpre...
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...
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...
On the surface of the Moon a large number of linear features are recognizable. Long and narrow depre...