MN of Plandl 20.00U tlmn that of Orbit: FIG. 4 . (Jupiter and Safum am chown In Marr tru: aria/pant/on, Uramn andlvleptuna in tha axial positron: /nferred /rom the motions of than Satellites /-Souls about 4000 times that of tha Orblts r Y /iF" E l 1 ' = 5 1 = 'i 8aturn's 3 7585/stem of Satellites 3 , / ggag; l lap/f, ,», }; Sym". 3 of s.¢¢~, m s ] Q s r ' J ' " " FIG. 5 In the figures given above are shown the relative orbits of the The relative siees of the planets are also given, orientated in their giancts, the orbits of Mars, the Earth, Venus and Mercury (fig. 1) true axial position with regard to the ecliptic. The nearer planets Ing draw n to a scale twenty times that of the outer ones-Neptune, (and also the Moon) are separately compared (fig. 3); and then shown Lranus, Saturn, Jupiter (fig 2). The pos1t1ons of the planets at (on a smaller scale) in comparison w1th the more distant ones ten-day mterx als; their actual position on the 1st of January 1910 at (fig. 4). Finally scale diagrams of the distances of the orbits of noon. of their nodes and nearer apses, and the points w en they the satellite systems of Satur U are farthest distant north and h ' sout of the ecliptic, are also given. - n, ranus, Iupiter and Neptune are

given (fig. 5).