In the 18th century, astronomers of the Academie des sciences of Paris made
various contributions to the improvement of navigation: terrestrial determ
inants of longitude which improved charts for navigators, testing of marine
clocks for longitude determinations at sea. They were also invited to join
exploratory voyages; such as d'Agelet, who accompanied Kerguelen and later
La Perouse. In order to resolve the Cassini-Newton controversy regarding t
he shape of the Earth, the Academie proposed, in 1735, that two expeditions
should be ,ade with a view to measuring a meridian arc: one in "Perou" clo
se to the equator (Godon, Bouger, La Condamine); the other in Lapland (Maup
ertuis, Clairaut). The results concluded that the Earth was flat on the sid
es of the poles, as predicted by Newton. By mid-18th century, the first pur
ely astronomical expedition (La Caille, Cape of Good Hope) led to the creat
ion of an austral celestial map and new parallaxes. Later, Clappe d'Auteroc
he, Le Gentil and Pingre travelled to observe two transits of Venus over th
e Sun (1761, 1769) for the improvement of the solar parallax. (C) Academie
des sciences/Elsevire, Paris.