Part II.—Satellites of Planets.
Part III.—Rings of Saturn.
| Rings. | Diameter of Rings in Miles. | Areas of Rings in Square Miles. | Thickness of Rings in Miles. | Volume of Rings in Cubic Miles. | Density (Water=1). | Volume at Density of Water in Cubic Miles. | |||
| Outer | ![]() | Outer | 172,240 | ![]() | 5,252,035,427 | ||||
| Inner | 151,590 | ||||||||
| Middle | ![]() | Outer | 148,100 | ![]() | 6,919,075,757 | ||||
| Inner | 114,560 | ||||||||
| Dark | ![]() | Outer | 110,060 | ![]() | 3,040,689,488 | ||||
| Inner | 90,993 | ||||||||
| Total | 15,211,800,672 | 90 | 1,369,062,060,480 | .0001425 | 195,000,000 | ||||
(4) All of these bodies, planets, satellites, and rings were supposed to revolve around their primaries, and to rotate on their axes, in the same direction viz., from right to left, in the opposite direction to the hands of a watch.
In addition to the above definition it is necessary to give some sort of description of the various parts of the machine or system which has to be made out of the nebula, with their positions, dimensions, and details. This we believe will be made plain enough, in the simplest manner, by [Table No. I]., taken and calculated from the elements of the solar system given in almost all astronomical works, from which we have selected what we believe to be the most modern data.
The construction of this table requires some explanation on account of its being made to show complete results from incomplete data. There has been no difficulty with the sun, the major planets, and the satellites of the earth and Jupiter, but for the minor planets, the satellites of the three outer planets, and the rings of Saturn, we have been obliged to exercise our judgment as best we could.
There being almost no data whatever of the dimensions and densities of the minor planets, to be found, we have been driven in order to assign some mass to them, to imagine the existence of one planet to represent the whole of them (in fact Olbers's planet before it exploded), which we have supposed to be placed at the mean distance of 260,300,000 miles from the centre of the sun; and we have given to it a mass equal to one-fourth of the mass of the earth, that being, in the opinion of some astronomers, the greatest mass which the whole of them put together could have. This assumption we shall explain more fully at a more suitable time.


