Rilles. All trenches on the Moon a called by this appellation, since we don't know exactly what caused them [ i. e. , plate tectonics , erosion , or other terms we use for cracks on Earth ] .
The long deep cracks in the Maria Bedrock on the Moon are called rilles. These are narrow, trench-like depressions that can be several kilometers wide and hundreds of kilometers long. Rilles are thought to have formed from a combination of volcanic and tectonic processes.
B. rilles. Rilles are long, narrow depressions on the Moon's surface that are typically formed by ancient lava flows or tectonic activity. They can appear as cracks in the bedrock when viewed from a distance.
The flat areas on the moon are called lunar maria. They are dark plains formed by ancient volcanic activity and are visible from Earth as dark patches on the moon's surface.
Dark places on the moon are called lunar maria, which are large, flat, dark-colored basaltic plains formed by ancient volcanic activity. These areas contrast with the brighter highlands on the moon's surface.
Low altitude areas on the moon are called maria, which are large dark plains formed by ancient volcanic activity. The maria are located on the side of the moon that faces Earth.
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.
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.
B. rilles. Rilles are long, narrow depressions on the Moon's surface that are typically formed by ancient lava flows or tectonic activity. They can appear as cracks in the bedrock when viewed from a distance.
Craters :P
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.
the light areas of the moon are called the highlands. the dark areas are called maria.
The flat areas on the moon are called lunar maria. They are dark plains formed by ancient volcanic activity and are visible from Earth as dark patches on the moon's surface.
cracks in the moon's icy surface
They are called seas.
The low areas of the moon are called "maria," which are large, dark basaltic plains created by ancient volcanic activity. These areas are lower in elevation compared to the moon's rugged and heavily cratered highlands.
Maria isn't a name of a moon, though it's what the dark areas on our own moon are called which were once though to be seas.
These dark flat areas are called lunar maria, which are large basaltic plains formed by ancient volcanic activity. They have lower elevation compared to the surrounding highlands and were formed billions of years ago by lava flows filling in large impact basins.
The dark smooth plains on the moon are called lunar maria. They are vast, flat areas formed by ancient volcanic activity. Maria is the Latin word for "seas," as they were once believed to be bodies of water.