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    Academy lesson

    Planetary science

    How planets differentiate, why atmospheres differ, and what geology tells us about history.

    Intermediate 10 min read
    MercuryVenusEarthMarsJupiterSaturnUranusNeptuneOrder from the Sun — sizes and distances not to scale

    Layered worlds

    As young planets heated up, dense iron sank to the centre and lighter rock floated up — a process called differentiation. Rocky planets have cores, mantles and crusts; giant planets have deep envelopes of hydrogen and helium around dense interiors.

    Atmospheres

    Whether a planet keeps an atmosphere depends on its gravity, temperature and magnetic protection. Venus has a crushing carbon dioxide atmosphere and a runaway greenhouse; Mars lost most of its air and is now cold and dry; Titan, a moon, has a thicker atmosphere than Earth.

    Reading surfaces

    Craters count time: older surfaces have more of them. Volcanoes, river channels, ice and tectonic features record a world's activity. Rovers analyse rocks directly, while orbiters map composition from spectra.

    Knowledge check

    1. Heavily cratered surfaces are generally:
    2. Which world has a runaway greenhouse atmosphere?