Planets are celestial bodies that orbit around a star, such as our Sun. They are typically large, spherical objects that do not produce their own light but instead reflect the light of the star they orbit. In our solar system, there are eight recognized planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
Each planet has its own unique characteristics, including size, composition, atmosphere, and surface features. Here are some key characteristics of the planets in our solar system:
Planets are believed to form from the same cloud of gas and dust that gives rise to a star. This process, known as planetary accretion, involves the gradual accumulation of material in a protoplanetary disk around the young star. Over time, the material clumps together to form planetesimals, which then collide and merge to form planets.
In our solar system, planets are classified into two main groups: terrestrial planets and gas giants. Terrestrial planets, including Mercury, Venus, Earth, and Mars, are small, rocky, and located closer to the Sun. Gas giants, such as Jupiter, Saturn, Uranus, and Neptune, are much larger and primarily composed of hydrogen and helium.