1 Moon
The Moon is Earth’s only natural satellite and the fifth-largest moon in the Solar System. It is the closest celestial body to Earth and the only extraterrestrial object humans have visited. The Moon plays a key role in shaping Earth’s tides, stabilizing its axial tilt, and inspiring scientific exploration and cultural significance throughout human history.
1.1 General Properties
1.2 Physical Characteristics
The Moon is a rocky, airless world with a heavily cratered surface shaped by billions of years of impacts. It has no global magnetic field and only a very thin exosphere composed of trace gases such as helium and neon.
The surface features include:
- Maria – dark basaltic plains formed by ancient volcanic activity.
- Highlands – older, brighter, heavily cratered regions.
- Craters – formed by meteorite impacts.
- Rilles – channels likely carved by ancient lava flows.
1.3 Internal Structure
The Moon has a differentiated structure:
- Crust – about 50 km thick on average, composed of anorthosite.
- Mantle – made of silicate rock, possibly still partially molten in places.
- Core – likely consists of iron and nickel, partially molten.
1.4 Orbit and Rotation
The Moon is tidally locked with Earth, meaning the same side (the near side) always faces Earth, while the far side remained unseen until spacecraft flew around it. Its synchronous rotation and orbital period are both ~27.3 days.
The Moon’s gravitational interaction with Earth causes ocean tides and gradually slows Earth's rotation while increasing the Moon’s orbital distance by about 3.8 cm per year.