Gas giants are believed to have formed farther from the sun where the lower temperatures allowed hydrogen and helium to condense into solidcores. These cores then attracted more gas and dust from the surrounding protoplanetary disk, eventually growing into the massive planets we see today.
Study Guide
Here are some key points to remember when studying gas giants:
What are the primary components of a gas giant's atmosphere?
Physics: Students will use scientific skills and processes to explain the interactions of matter and energy and the energy transformations that occur.
Thermodynamics: Identify and explain that heat energy is a product of the conversion of one form of energy to another.
Identify and describe the various forms of energy that are transformed in order for systems (living and non-living) to operate: Chemical - Flashlight-Light; Mechanical - Pulleys-Motion; Solar/Radiant - Solar calculator; Chemical - Plant cells.