The surface of the moon, often referred to as the 'lunar surface', is quite unique compared to that of Earth. Unlike Earth, which has a dynamic surface shaped by water and atmospheric movements, the moon's surface is almost static. This stillness is due to the absence of an atmosphere. The lunar surface is covered with a layer of fine dust and rocky debris called 'regolith'.
The lack of weather on the moon means that any marks, like the footprints left by astronauts during the Apollo missions, remain virtually unchanged. It is this lack of change that allows such footprints and other disturbances to remain visible for millions of years.
The lunar surface is also filled with many craters caused by meteorite impacts due to the lack of an atmosphere to burn up incoming objects.
Key features of the lunar surface include:
- Regolith – fine dust and rocky debris
- Meteorite Craters
- Rilles – long, narrow depressions or valleys