1. The solar system evolved from an enormous rotating cloud called the solar nebula
2. The nebula was composed mostly of hydrogen and helium
3. 5 billion years ago, the nebula began to contract
4. It assumed a flat, disk shape with the protosun (pre-Sun) at the center
5. Inner planets begin to form metallic and rocky clumps
6. Larger outer planets began forming from fragments with a high percentage of ice