The Moon is Earth's only proper natural satellite. It is one-quarter the diameter of Earth (comparable to the width of Australia), making it the largest natural satellite in the Solar System relative to the size of its planet.
It is the fifth largest satellite in the Solar System and is larger than any dwarf planet. The Moon orbits Earth at an average lunar distance of 384,400 km (238,900 mi), or about 30 times Earth's diameter. Its gravitational influence produces Earth's tides and slightly lengthens Earth's day.
The Moon is classified as a planetary-mass object and a differentiated rocky body. It lacks any significant atmosphere, hydrosphere, or magnetic field, and its surface gravity is about one-sixth of Earth's (0.1654 g). Jupiter's moon Io is the only satellite in the Solar System known to have a higher surface gravity and density.
The Moon is tidally locked to Earth, which means that the length of a full rotation of the Moon on its own axis (a lunar day) is the same as the synodic period, resulting in its same side (the near side) always facing Earth. The Moon's apparent size is nearly the same as that of the Sun, allowing it to cover the Sun almost completely during a total solar eclipse.
Near side of the Moon
The near side of the Moon is marked by dark volcanic maria ("seas"), which fill the spaces between bright ancient crustal highlands and prominent impact craters. The lunar surface is relatively non-reflective, with a reflectance just slightly brighter than that of worn asphalt. However, because it reflects direct sunlight, is contrasted by the relatively dark sky, and has a large apparent size when viewed from Earth, the Moon is the brightest celestial object in Earth's sky after the Sun.
Crescent Moon
Earthshine
Equipment:
127Mak (F7.4 ) @ ISO100 for 1 second
EOS 600D on EQ5 Pro