Continent
Primeval Continents
Over four billion years ago, before the first continents developed, the mantle was much hotter than today. Accordingly, the rate of plate tectonics was much faster. This meant that plates were smaller, thinner and much warmer when subducted. The associated crust was nearer to its melting point and so partially melted along with the mantle. Early subduction zone volcanism therefore produced magmas with higher silica content, since partially melting basalt produces an intermediate magma composition. The early Earth consequently developed volcanic island arcs with relatively low density, which resisted subduction. These formed Earth's earliest micro-continents and built the first cratons when sutured together at subduction zones. Throughout the 1990s, research focused on early continent development and the questions of when continents first appeared, how they originated and at what rate growth occurred.
Resources
Books
Trefil, James. Meditations At 10,000 Feet: A Scientist In The Mountains. New York: Macmillan Publishing Company. 1986.
Vogel, Shawna. Naked Earth: The New Geophysics. New York: Penguin Books. 1995.
Periodicals
Taylor, S. Ross, and Scott McLennan. "The Evolution of Continental Crust." Scientific American (January 1996).
Weiss, Peter. "Land Before Time." Earth (February 1998).
Clay Harris
Additional topics
Science EncyclopediaScience & Philosophy: Condensation to CoshContinent - Crusts Compared, Continental Margins, Crustal Origins, Growing Pains, Primeval Continents - Structure of a continent