This book presents an exploration of the potential diversity of rocky planets through a quantitative study of how planetary processes change as properties deviate from the Earth. Changes in four specific properties are considered: the presence of a magnetic field, the production and loss of internal heat, planetary composition and volatile abundance. This is an interdisciplinary venture, with each chapter examining the variation found in the planets we can explore in-situ within our solar system and the expectation of how these properties may differ - and the resulting outcomes - across the broader range of the exoplanet population. This book will be of great interest to astrophysicists and planetary scientists focusing on exoplanets. In particular, graduate students and researchers.
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