Historical models of the solar system are efforts made by scientists over hundreds of years to understand our solar system. The solar system is the collection of planets, moons, asteroids, and other objects that orbit around the sun.
In the early days, people thought that the Sun, Moon, and stars revolved around Earth. They thought that the universe was small and could fit in a dome or bowl. Over time, people started to learn more about the night sky and realized that this wasn't true.
After studying the stars, people figured out that the Sun, Moon, and planets all revolved around Earth. Then, in the 1600s, a scientist named Johannes Kepler suggested that the planets might actually go around the Sun instead. He thought that all the planets moved in their own orbit around the Sun, in an order from innermost to outermost.
It took a while for people to accept this new idea, but eventually it was accepted. In the 1800s, scientists started proposing different models of what the orbits and sizes of the objects in the solar system might be. Each model tried to explain more, like why the planets have different sizes and distances from the Sun, and why they move at different speeds.
These models have allowed us to learn a lot more about the solar system--not just what the objects look like to us on Earth, but also how they interact with each other, and even where new objects might be hiding in space.