ii i a ic fluid as it is now, but of Monf. Cajfini s 
and the laft as ^ • the Confequence. Since in that 
Figure, and » , ^ r than the Equatorial 
Figure the Axi _ ,z fo fflUch greater at the 
Diameter^ the Gravity ^ ^ Wat£rs wiU aU flow 
and I lin V vefyw P el! : awK* be objected by fudi 
38 dSir "l^N^oTsTrSci^^ have not read 
read Sir ljaac « That 1 have not ar- 
« au rffeS '^drawing Confequences from a greater 
gued tair y t h an at the Poles, in an ob- 
“ £nt V SaheroW fbecaufe Monf. Matran has (hewn, 
Sr* £» . - to 1 “r' d - 
s“ ssssstxt 
a |»«. 7 ,: f & cL° f 
Curvature drawn into the Perpendicular to the Curve, , 
terminated at the Axis ; let us confider what will follow 
ft TLet uSnfoppofe the Earth at nrft in a fluid 
State- A A the Axis, M the Equatorial Diameter a A U 
Ray of Curvature, in another, and ^Ctwo Lines 
* Fig. II* 
of 
