摘要
One of the central and most vivid problems of celestial mechanics in the 18th and 19th centuries was the motion description of the Sun-Earth-Moon system under the Newtonian gravitation field（Figure 1（a））.Notable work was done by Euler（1760）,Lagrange（1776）,Laplace（1799）,Hamilton（1834）,Liouville（1836）,Jacobi（1843）,and Poincar′e（1889）[1]and Xia（1992）[2].
One of the central and most vivid problems of celestial mechanics in the 18th and 19th centuries was the motion description of the Sun-Earth-Moon system under the Newtonian gravitation field(Figure 1(a)).Notable work was done by Euler(1760),Lagrange(1776),Laplace(1799),Hamilton(1834),Liouville(1836),Jacobi(1843),and Poincar′e(1889)[1]and Xia(1992)[2].The study of the motion between
