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Hello,
A student asked me this question in class yesterday, and I wasn't sure
(haven't looked at the Principia in a long time, but always found the
arguments a bit hard to follow). I imagine he could do it from a rough
estimate of the mass of the Earth, mass of the Moon, and distance to the
Moon. With the Moon's period you could get a value for G. Is this how he
did it? I know that the direct measurement wasn't done until later, by
Cavendish.
Further, did he have any way of estimating the distance to the Sun? I
couldn't think of one that was available at his time, but he was more clever
than I. :)
thanks,
bb
--
Brian Blais
bblais@bryant.edu
http://web.bryant.edu/~bblais <http://web.bryant.edu/%7Ebblais>
http://bblais.blogspot.com/
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