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Lesson 2.2 – The Inner Rocky Planets

16 Dec 2025 Module 2: Our Solar System
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Part of a Module

This lesson is part of Module 2: Our Solar System. Take it in course mode for progress tracking and the end-of-module exam.

What Are the Inner Planets?

The inner planets — Mercury, Venus, Earth, and Mars — are called terrestrial planets. They are:

  • Small

  • Dense

  • Made mostly of rock and metal

  • Located close to the Sun


Mercury – The Extreme World

  • Closest planet to the Sun

  • No significant atmosphere

  • Temperatures range from -180°C to 430°C

  • A year lasts just 88 Earth days


Venus – Earth’s Twin Gone Wrong

  • Similar size to Earth

  • Thick carbon dioxide atmosphere

  • Surface temperature ~465°C

  • Crushing atmospheric pressure

Venus demonstrates what a runaway greenhouse effect looks like.


Earth – The Goldilocks Planet

Earth sits in the habitable zone, where liquid water can exist.

Key features:

  • Liquid oceans

  • Protective magnetic field

  • Stable atmosphere

  • Active geology


Mars – The Red Planet

  • Cold, thin atmosphere

  • Evidence of ancient rivers and lakes

  • Home to Olympus Mons (largest volcano)

  • Target for future human missions


Key Takeaways

  • Inner planets are rocky and dense

  • Earth is uniquely balanced

  • Mars holds clues to past habitability

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