THE PLANETS AS INDIVIDUALS.

"Through faith we understand that the worlds [plural] were framed

by the word of God, so that things which were seen were not made

of things which do appear."--_Heb._ xi. 3.

[Page 136]

"O rich and various man! Thou palace of sight and sound, carrying

in thy senses the morning, and the night, and the unfathomable

galaxy; in thy brain the geometry of the city of God; in thy heart

the power of love, and the realms of right and wrong. An individual

man is a fruit which it costs all the foregoing ages to form and

ripen. He is strong, not to do but to live; not in his arms, but

in his heart; not as an agent, but as a fact."--EMERSON.

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VII.

_THE PLANETS AS INDIVIDUALS._

How many bodies there may be revolving about the sun we have no

means to determine or arithmetic to express. When the new star

of the American Republic appeared, there were but six planets

discovered. Since then three regions of the solar system have been

explored with wonderful success. The outlying realms beyond Saturn

yielded the planet Uranus in 1781, and Neptune in 1846. The middle

region between Jupiter and Mars yielded the little planetoid Ceres

in 1801, Pallas in 1802, and one hundred and ninety others since.

The inner region between Mercury and the sun is of necessity full

of small meteoric bodies; the question is, are there any bodies

large enough to be seen?

The same great genius of Leverrier that gave us Neptune from the

observed perturbations of Uranus, pointed out perturbations in

Mercury that necessitated either a planet or a group of planetoids

between Mercury and the sun. Theoretical astronomers, aided by the

fact that no planet had certainly been seen, and that all asserted

discoveries of one had been by inexperienced observers, inclined

to the belief in a group, or that the disturbance was caused by

the matter reflecting the zodiacal light.

When the total eclipse of the sun occurred in 1878, [Page 138]

astronomers were determined that the question of the existence of an

intra-mercurial planet should be settled. Maps of all the stars in

the region of the sun were carefully studied, sections of the sky

about the sun were assigned to different observers, who should

attend to nothing but to look for a possible planet. It is now

conceded that Professor Watson, of Ann Arbor, actually saw the

sought-for body.

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