which they severally belong, as may be seen by the assist- ance of the telescope. The Sun is the center round which those six worlds or planets revolve at different distances therefrom, and in circles concentric to each other. Each world keeps constantly in nearly the same tract round the Sun, and continues at the same time turning round itself, in nearly an upright position, as a top turns round itself when it is spinning on the ground, and leans a little sideways. It is this leaning of the earth (23½ degrees) that occasions summer and winter, and the different length of days and nights. If the earth turned round itself in a position per- pendicular to the plane or level of the circle it moves in round the Sun, as a top turns round when it stands erect on the ground, the days and nights would be always of the same length, twelve hours day and twelve hours night, and the season would be uniformly the same throughout the year. Every time that a planet (our earth for example) turns round itself, it makes what we call day and night; and every time it goes entirely round the Sun, it makes what we call a year, consequently our world turns three hundred and sixty-five times round itself, in going once round the Sun. * The names that the ancients gave to those six worlds, and which are still called by the same names, are Mercury, Venus, this world that we call ours, Mars, Jupiter, and Saturn. 1 They appear larger to the eye than the stars, being many million miles nearer to our earth than any of the stars ____________________ | * | Those who supposed that the Sun went round the earth every 24 hours made the same mistake in idea that a cook would do in fact, that should make the fire go round the meat, instead of the meat turning round itself towards the fire. -- Author. | | 1 | With reference to the omission of any mention of Uranus, see the Introduc- tion. In the New York edition, 1794, edited by Col. John Fellows, occurs this footnote: "Mr. Paine had made no mention of the planet Herschel, which was first discovered, by the person whose name it bears, in 1781. It is at a greater distance from the Sun than either of the other planets and consequently occupies a greater length of time in performing its revolutions." -- Editor. | -69- |