Recreations in Astronomy eBook

This eBook from the Gutenberg Project consists of approximately 235 pages of information about Recreations in Astronomy.

Recreations in Astronomy eBook

This eBook from the Gutenberg Project consists of approximately 235 pages of information about Recreations in Astronomy.

Intermingled with these currents of air are the currents of electric power, all derived from the sun.  These have shown their swiftness and willingness to serve man.  The sun’s constant force displayed on the earth is equal to 543,000,000,000 engines of 400-horse power each, working day and night; and yet the earth receives only 1/21500000000 part of the whole force of the sun.

Besides all this, the sun, with provident care, has made and given to us coal.  This omnipotent worker has stored away in past ages an inexhaustible reservoir of his power which man may easily mine and direct, thus releasing himself from absorbing toil.

EXPERIMENTS.

Any one may see the spots on the sun who has a spy-glass.  Darken the room and put the glass through an opening toward the sun, as shown in Fig. 37.  The eye-piece should be drawn out about half an inch beyond [Page 96] its usual focusing for distant objects.  The farther it is drawn, the nearer must we hold the screen for a perfect image.

By holding a paper near the eye-piece, the proper direction of the instrument may be discovered without injury to the eyes.  By this means the sun can be studied from day to day, and its spots or the transits of Mercury and Venus shown to any number of spectators.

[Illustration:  Fig. 37.—­Holding Telescope to see the Sun’s Spots.]

First covering the eyes with very dark or smoked glasses, erect a disk of pasteboard four inches in diameter between you and the sun; close one eye; stand near it, and the whole sun is obscured.  Withdraw from it till the sun’s rays just shoot over the edge of the disk on every side.  Measure the distance from the eye to the disk.  You will be able to determine the distance of the sun by the rule of three:  thus, as four inches is to 860,000 miles, so is distance from eye to disk to distance from disk to the sun.  Take such measurements at sunrise, noon, and sunset, and see the apparently differing sizes due to refraction.

[Page 97] VI.

THE PLANETS, AS SEEN FROM SPACE.

“He hangeth the earth upon nothing.”—­Job xxvi. 7.

[Page 98] “Let a power be delegated to a finite spirit equal to the projection of the most ponderous planet in its orbit, and, from an exhaustless magazine, let this spirit select his grand central orb.  Let him with puissant arm locate it in space, and, obedient to his mandate, there let it remain forever fixed.  He proceeds to select his planetary globes, which he is now required to marshal in their appropriate order of distance from the sun.  Heed well this distribution; for should a single globe be misplaced, the divine harmony is destroyed forever.  Let us admit that finite intelligence may at length determine the order of combination; the mighty host is arrayed in order.  These worlds, like fiery coursers, stand waiting the command to fly.  But, mighty spirit, heed well the grand step, ponder well the

Copyrights
Project Gutenberg
Recreations in Astronomy from Project Gutenberg. Public domain.