By George Howard Darwin
Publisher: Cambridge University Press
Print Publication Year:2009
Online Publication Date:September 2010
Original Publication Year:1908
Subjects: Planetary Science , Astronomy: general interest
Sir George Darwin (1845–1912) was the second son and fifth child of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His family home is now the location of Darwin College. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). He also developed a theory of evolution for the Sun–Earth–Moon system based on mathematical analysis in geophysical theory. This volume of his collected papers covers tidal friction and cosmogony.
TIDAL FRICTION AND COSMOGONY
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