AstronomyLesson 1 of 1 in the course The Big Bang
Inflation and the Early Universe: Puzzles, Forces, and Evidence
5 flashcards · 5 quiz questions · 5 match pairs · 5 fill-in sentences · English
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Summary
The hot Big Bang model successfully explains the expansion of the universe, the cosmic microwave background (CMB), and the abundance of light elements. Yet it leaves important questions about the universe as a whole unanswered. This lesson introduces two major puzzles: why the universe has critical density and why the CMB has nearly the same temperature in every direction.
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Based on Astronomy 2e by Andrew Fraknoi, David Morrison, Sidney Wolff (OpenStax), licensed CC BY 4.0. Adapted into a summary, flashcards and quizzes.
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