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The Evolution of Modern Continents,own in Fig. 3.1. While it is unlikely to have produced the majority of the early continents, this process could have played a role in areas where mantle motion carried young continental fragments around the surface of the young Earth.
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Plate Tectonics, Planetary Magnetism and Life,d’s erosive flow from the outskirts of our atmosphere. In this chapter, we examine how such a field comes about; whether the Earth has always had it; and whether a planet can still be habitable without one.
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Mountains, Atmosphere and Long-Term Habitability,onnection between what is happening on the surface of a planet and the stability of this gaseous sea. We can infer this gaseous ocean’s composition from its geological activity and vice versa, allowing us to make testable predictions about the atmospheres of planets far removed from the Earth.
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