Moon

The moon is the fifth largest natural satellite in the solar system, with a diameter just under the width of China. It's composed of an iron-rich core, plus a mantle and crust containing minerals made of magnesium, oxygen and silicon. The moon's surface was once geologically active and covered in an ocean of magma. But today, apart from traces of water ice, the surface is completely covered in dust and rocky debris. Countless craters dot the moon's surface. Each is formed by objects such as meteoroids, comets and asteroids crashing onto the moon. The largest crater, the South Pole Aitkin basin, spans across a quarter of the moon's surface and is nearly deep enough to fit Mount Everest inside. The moon orbits our planet at an average distance of 30 Earths. It rotates at the same rate that it revolves. So as it revolves around our planet, the same side of the moon faces the Earth at all times. From the Earth's surface, we can observe eight distinct traditionally recognised stages of the moon's illumination, called lunar phases. They have been observed for thousands of years, and even provided the basis for the earliest calendars.