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PLANETS It will be observed that the distance from the sun is given in terms of the distance of the earth as a unit. The relative sizes of the planets and the sun are well-shown in the accompanying figure:

For the laws which describe the motion of the planets about the sun see and.

Concerning the individual planets it may be noted that



1., which is nearest the sun, has the least diameter, the least mass and the greatest density of all the planets. Its density may be remembered from the fact that it is almost exactly that of the metal mercury, being 12½ times that of water. The diameter of this planet is about 3,000 miles. No has been discovered for Mercury.

2. has a diameter of 7,700 miles and a density 0.86 that of Earth, so that in size, surface, gravity she is not very different from our own planet. No satellite is known.

3. . See.

4. has a diameter of 4,200 miles, and a density which is 0.73 that of Earth, so that bodies at the surface of Mars weigh only 0.38 what they would at the surface of Earth. Two satellites of this planet were discovered by Professor Hall at Washington in August, 1877. These two moons, Deimos and Phobos, are exceedingly minute, being only 7 and 5 miles, respectively, in diameter. The surface of Mars is covered with interesting markings.

5. . See.

6., the largest of all planets, has a diameter of 86,500 miles; and, while its density is only one quarter that of Earth, its mass is 316 times as great, so that a body on the surface of Jupiter weighs more than twice as much as the same body at the surface of Earth. The surface of this planet exhibits some very characteristic markings, especially belts and spots, which lead to the opinion that Jupiter is a body of very high temperature compared with the other planets. He has five satellites, four discovered by Galileo and one by Barnard in 1892 at Lick Observatory.

7., with its system of rings, is conceded to be one of the most superb objects in the heavens. Although the diameter of the planet is only 73,000 miles, the outer ring is no less than 168,000 miles across. Two rings had been known for a long while, but the third ring was discovered by Bond in 1850. Pierce and Maxwell have proved that these rings are made up of discrete particles and that the rings, therefore, are neither solid nor liquid. See. Saturn has eight satellites discovered between 1665 and 1848.

8., discovered by the older Herschel, has a diameter of 32,000 miles; but its density is only about one fifth that of Earth, so that, notwithstanding its enormous bulk, surface gravity there is only 0.90 that of Earth. It is accompanied by four satellites.

9., the most distant member of the family has a diameter of 35,000 miles and a density one fifth that of Earth. At an average distance of 2,800 millions of miles from the sun, it is absolutely invisible at Earth, except by the aid of a. It has one satellite, discovered almost immediately after the discovery of the planet itself. See Miss Clerke’s History of Astronomy and Chambers’ Descriptive and Practical Astronomy.  Plant′-Breeding, a term covering several processes of improving varieties of plants or of producing new varieties. It is done by selection or by crossing. Its purpose may be to produce fruits that are better flavored, to produce larger yields or to produce plants that are more resistant to disease, to pests or unfavorable climatic conditions. Selection is simply using such material for “seed” as to a greater or less degree shows the desired trait; or it is