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?
Reading Standards for Literacy in Science and Technical Subjects
Craft and Structure
Determine the meaning of symbols, key terms, and other domain-specific words and phrases as they are used in a specific scientific or technical context relevant to grades 6-8 texts and topics.