We know that the Sun is the host star of our solar system and that eight planets and other objects such as dwarf planets, asteroids, and comets orbit the Sun. In addition, some of the planets have moon(s) and rings orbiting around them.
But have you ever thought about these questions?
Curious to explore our amazing solar system? Let us find out the meaning of ‘solar’, first.
A planetary system consists of several planets revolving around a host star or a couple of host stars (as is commonly the case). The Sun is the lone host star of our planetary system. In Greek, the word ‘Solis’ refers to the Sun. Therefore, our planetary system is known as solar system. And anything related to the Sun is solar.
Our host star the Sun is a medium-sized star, and it is one of the 100 billion or more stars in our Milky Way galaxy. As per an estimate, the universe may contain two trillion such galaxies!!
Our solar system formed about 4.6 billion years ago from interstellar gas. This interstellar gas, over a lengthy period of time, clumped together to form a disk of rotating solar nebula. When the solar nebula collapsed to its center due to gravity, the center of the nebula became so dense and so hot that nuclear fusion got ignited. And the Sun was born.
The remaining rotating islands of clouds coalesced to form the planets around the Sun. Heavier content of the clouds withstood the solar wind and heat from the Sun and stayed in the inner orbits while the gaseous part of the cloud got pushed to the outer orbits. Therefore, the solar system has rocky terrestrial planets with metallic core in orbits closer to the Sun while the gaseous giant planets are far away from the Sun.
Here are a few key evidences that support the nebular hypothesis:
Information and data, in this post, are based on the following sources: