Popular lectures on scientific subjects : $b Second series, with an autobiography of the authorHelmholtz, Hermann von
Science
Popular lectures on scientific subjects : $b Second series, with an autobiography of the author
Helmholtz, Hermann von
Science; Universities and colleges -- Germany
traces of incipient fusion; and in cases in which observers examined
with sufficient promptitude the stones which had fallen they found them
hot on the surface, while the interior of detached pieces seemed to
show the intense cold of cosmical space.
To the individual observer who casually looks towards the starry
sky the meteorites appear as a rare and exceptional phenomenon. If,
however, they are continuously observed, they are seen with tolerable
regularity, especially towards morning, when they usually fall. But
a single observer only views but a small part of the atmosphere; and
if they are calculated for the entire surface of the earth it results
that about seven and a half millions fall every day. In our regions of
space, they are somewhat sparse and distant from each other. According
to Alexander Herschel’s estimates, each stone is, on an average, at a
distance of 450 miles from its neighbours. But the earth moves through
18 miles every second, and has a diameter of 7,820 miles, and therefore
sweeps through 876 millions of cubic miles of space every second, and
carries with it whatever stones are contained therein.
Many groups are irregularly distributed in space, being probably
those which have already undergone disturbances by planets. There are
also denser swarms which move in regular elliptical orbits, cutting
the earth’s orbit in definite places, and therefore always occur on
particular days of the year. Thus the 10th of August of each year is
remarkable, and every thirty-three years the splendid fireworks of the
12th to the 14th of November repeats itself for a few years. It is
remarkable that certain comets accompany the paths of these swarms, and
give rise to the supposition that the comets gradually split up into
meteoric swarms.
This is an important process. What the earth does is done by the other
planets, and in a far higher degree by the sun, towards which all the
smaller bodies of our system must fall; those, therefore, that are
more subject to the influence of the resisting medium, and which must
fall the more rapidly, the smaller they are. The earth and the planets
have for millions of years been sweeping together the loose masses in
space, and they hold fast what they have once attracted. But it follows
from this that the earth and the planets were once smaller than they
are now, and that more mass was diffused in space; and if we follow
out this consideration it takes us back to a state of things in which,
perhaps, all the mass now accumulated in the sun and in the planets,
wandered loosely diffused in space. If we consider, further, that the
small masses of meteorites as they now fall, have perhaps been formed
by the gradual aggregation of fine dust, we see ourselves led to a
primitive condition of fine nebulous masses.
From this point of view, that the fall of shooting-stars and of
meteorites is perhaps only a small survival of a process which once
built up worlds, it assumes far greater significance.
Public-domain text, read in full here on John Shaqi.
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