Maria
Trenches on the moon are called rilles, and they are thought to be long, narrow depressions carved by lava flows or collapsed lava tubes. Rilles can stretch for hundreds of kilometers across the lunar surface, providing clues to the moon's volcanic past and geologic history. These features are a common and intriguing aspect of the moon's landscape.
Rilles. Rilles are long, narrow depressions on the Moon's surface, often found in lunar maria. They can be several kilometers wide and hundreds of kilometers long, thought to have been formed by ancient lava flows or collapsing lava tubes.
Some landforms found on the moon that Earth does not have include impact craters of various sizes, such as lunar mare basins and rays, formed by meteoroid impacts. Additionally, the moon features lava tubes and rilles, which are long, deep valleys formed by ancient volcanic activity.
Young craters are often associated with features like sharp rims, well-defined ejecta blankets, and a relatively fresh appearance due to the lack of weathering or erosion. These features indicate that the crater was formed relatively recently in geological terms.
The canyons on the moon are known as rilles. They are thought to have been created by ancient volcanic activity or by the collapse of lava tubes. Rilles can sometimes stretch for hundreds of kilometers across the lunar surface.
Ridges, rilles, craters and regoliths
Cracks in the moon's bedrock are called "faults" or "fractures." These features are caused by stress and movement within the lunar surface, much like on Earth.
Trenches on the moon are called rilles, and they are thought to be long, narrow depressions carved by lava flows or collapsed lava tubes. Rilles can stretch for hundreds of kilometers across the lunar surface, providing clues to the moon's volcanic past and geologic history. These features are a common and intriguing aspect of the moon's landscape.
Rilles. Rilles are long, narrow depressions on the Moon's surface, often found in lunar maria. They can be several kilometers wide and hundreds of kilometers long, thought to have been formed by ancient lava flows or collapsing lava tubes.
Maria, terrae and sinuous rilles.
Some landforms found on the moon that Earth does not have include impact craters of various sizes, such as lunar mare basins and rays, formed by meteoroid impacts. Additionally, the moon features lava tubes and rilles, which are long, deep valleys formed by ancient volcanic activity.
Young craters are often associated with features like sharp rims, well-defined ejecta blankets, and a relatively fresh appearance due to the lack of weathering or erosion. These features indicate that the crater was formed relatively recently in geological terms.
The canyons on the moon are known as rilles. They are thought to have been created by ancient volcanic activity or by the collapse of lava tubes. Rilles can sometimes stretch for hundreds of kilometers across the lunar surface.
Those features are called rilles, which are long, narrow valleys on the surface of the Moon. They can be several kilometers wide and hundreds of kilometers long, and are thought to have been formed by ancient lava flows or tectonic activity.
The deep narrow valleys on the Moon are called rilles. These are long, winding depressions that can stretch for many kilometers across the lunar surface. Rilles are thought to have been formed by a combination of ancient volcanic activity and tectonic forces.
Craters are one of the moon's landforms. Another lunar landform is a maria, which is what Galileo called the lowland areas of the moon because he thought that they were covered in water (maria is Latin for sea).
Another name for a lunar valley is a rille. These are long, narrow depressions on the moon's surface that can be several kilometers wide and hundreds of kilometers long. Rilles are believed to have formed through a combination of volcanic and tectonic processes.