Gas giants are a type of planet that are primarily composed of hydrogen and helium, with a small rocky core at their center. They are also known as Jovian planets, named after Jupiter, the largest gas giant in our solar system.
The four gas giants in our solar system are:
Gas giants are believed to have formed farther from the sun where the lower temperatures allowed hydrogen and helium to condense into solid cores. These cores then attracted more gas and dust from the surrounding protoplanetary disk, eventually growing into the massive planets we see today.
Here are some key points to remember when studying gas giants:
Understanding gas giants is essential for grasping the diversity of planetary systems and the processes involved in planetary formation.