Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
Interest in a possible planet or planets outside the orbit of Neptune is
likely to increase rather than diminish. To the ancients seven was the
perfect number, there were seven heavenly bodies already known, so there
could be no use whatever in looking for an eighth. The discovery of
Uranus in 1781 proved the futility of such logic, and Neptune followed
in 1846 with further demonstration, if need be. The cosmogony of the
present day sets no outer limit to the solar system, and some
astronomers advocate the existence of many trans-Neptunian planets.
CHAPTER XL
COMETS--THE HAIRY STARS
Comets--hairy stars, as the origin of the name would indicate--are the
freaks of the heavens. Of great variety in shape, some with heads and
some without, some with tails and some without, moving very slowly at
one time and with exceedingly high velocity at another, in orbits at all
possible angles of inclination to the general plane of the planetary
paths round the sun, their antics and irregularities were the wonder and
terror of the ancient world, and they are keenly dreaded by
superstitious people even to the present day.
Down through the Middle Ages the advent of a comet was regarded as:
Threatening the world with famine, plague and war;
To princes, death; to kingdoms, many curses;
To all estates, inevitable losses;
To herdsmen, rot; to plowmen, hapless seasons;
To sailors, storms; to cities, civil treasons.
Comets appeared to be marvelous objects, as well as sinister, chiefly
because they bid apparent defiance to all law. Kepler had shown that the
moon and the planets travel in regular paths--slightly elliptical to be
sure, but nevertheless unvarying. None of the comets were known to
follow regular paths till the time of Halley late in the seventeenth
century, when, as we have before told, a fine comet made its
appearance, and Halley calculated its orbit with much precision.
Comparing this with the orbits of comets that had previously been seen,
he found its path about the sun practically identical with that of at
least two comets previously observed in 1531 and 1607.
So Halley ventured to think all these comets were one and the same body,
and that it traveled round the sun in a long ellipse in a period of
about seventy-five or seventy-six years. We have seen how his prediction
of its return in 1758 was verified in every particular. On the comet's
return in 1910, Crowell and Crommelin of Greenwich made a thorough
mathematical investigation of the orbit, indicating that the year 1986
will witness its next return to the sun.
Public-domain text, read in full here on John Shaqi.
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