The features of the Moon were first mapped in the 17th century. The names of tens of thousands of craters were first assigned then. We can introduce some terms that are used to describe the features seen on the surfaces of other worlds. Craters, of course, are circular depressions on the surface. Here is a simulation of how they are made.Then there are the 3 r’s:Rays are streaks formed when material is ejected from an impact. Tycho has an extensive ray system around it.Rilles are stream-like features apparently formed by lava flow. They are found primarily in the mare regions.Regolith is the surface material of the Moon. It is the powdery ‘soil’ we see clinging to the boots of Apollo astronauts.
CratersCraters are circular depressions on the surface of an object caused, for the most part, by impacts. There are thousands of named craters on the Moon’s surface. They range is size from microscopic to several hundred kilometers in diameter. The interior walls of craters sometimes show a feature called terracing. One of the best examples of this is seen in the crater Langrenus.
RaysRays are evidence of impacts on the Moon. It is one component of the ‘ejecta blanket’ that surrounds a crater. The crater Tycho has a particularly impressive system of rays. Since the features are relatively shallow, they are usually only found around relatively young craters. Otherwise, the constant gardening of the surface by micrometroroid impacts would have erased them.
RillesAlso called sinuous rilles, these features look like rivers or streams, but are not caused by water flow. They are thought to originate as lava flows across the surface. We have analogous features called lava tubes here on Earth. The Apollo 15 crew landed right near the edge of Hadley Rille on the Moon in the summer of 1971.
RegolithRegolith is the ‘soil’ of the Moon. Technically not soil, since it has no organic components. It is formed when small meteoroids grind up the surface material. It is estimated that the regolith increases in depth by about a millimeter every million years. Other objects in the solar system have their own version of regolith on their surfaces with varying chemical compositions.