This document provides an overview of the history of astronomy and the current understanding of the solar system. It describes how models have progressed from Ptolemy's geocentric view to the acceptance of Copernicus' heliocentric model supported by Galileo's observations of phases of Venus and moons orbiting Jupiter. Newton later explained gravity and inertia as the forces that cause objects to remain in orbit. The document outlines the definition of planets and characteristics of the inner and outer planets, as well as how the solar system formed from a nebula 4.6 billion years ago. Minor objects like comets, asteroids, and meteoroids are also briefly described.