The Bottineau pioneer. (Bottineau, N.D.) 1885-1895, 1893-11-18
MlssiLEs FROM THE HEAVENS.
Billions Of Them Fall, but Compasstfv
Few Raach th~ Eo r%br

Billions Of Them Fall, but Comparatively
Few Reach the Earth.
ut is mistake to suppose that NETS
orites burst in the proper sense Of the
word" said scientist to writer. "But
1t often happens that they are broken to
pieces on striking the atmosphere of the
earth. This may seem surprising, bat
let me call your attention to an analogy.
6trike the surface Of water with your
fist, and, though fluid, the resistance it
opposes to the blow seems almost ~
strong as if it were solid. Now, the me.
teorite is moving at a tremendous rate Of
speed. If small, it is set on fire in an in
slant by the friction of the air, and after
glowing for moment brightly is con-
sumed.
ION any night in summer you will
see shooting stars now and then. They
are meteorites, which on coming into
contact with the earth's atmosphere are
set afire. This is not surprising, mas
much as they approach the planet on
which we live at speed which often at
tains A miles q second. By causing tho
destruction of meteorites the atmosphere
serves as protection for people on the
globe, who would otherwise be pelted
by such missiles to a dangerous extent.
It is estimated that not less than IL, ,OOO,.
600 Of them, big enough to be visible to
the naked eye, strike tho earth every "a
hours.
"By contact with this planet the me-
teorites are raised to temperature which
reaches from 100000 to 10000 de-
grees-high enough to consume the hard
est known substance almost instantly.
Thus only those of large size reach the
earth before being entirely burned up.
The greatest number of such bodies can
be seen just before daybreak, because by
that time we are on the front side Of tho
globe as it moves through space. The
elevation at which most Of them are Wis
ible has been found to be between As and
80 miles, very few being seen at greater
height than 100 miles.
1T is believed by most astronomers
that some very large meteors have en-
tered our atmosphere and have passed
out into space again, their great mo-
mentum being sufficient to take them
away from the earth's attraction. What
these flying bodies are is a question that
has been much disputed, but it il con-
sidered most likely that they are the
debris of broken up comets. In one re-.
cent instance the correctness Of this the
ory has found striking proof. That was
the case of the comet Of Biela. It was
discovered in 1925 and was again oh:
served in 1882, 1G IS and 1852. In 1S45 it
had split into two parts, and in 1879 1t
failed to appear when and where 1t
should have done. Evidently it had been
smashed up, and prediction was made
that there would be great meteoric
shower composed OF the rennsinB ef tho
lost comet. This prediction was fulfilled
'Certain groups Of meteors move In
elliptical orbits around the sun. Occa-
sionally the earth passes through their
clusters, producing what are known as
meteoric showers. Such showers occur
annually from the 9th to the 18th Of Al
gust, and there is similar display ir
November once every So years. The
stream of the August meteors is esti
mated to be from s, 900 900 to 10, ,000, 600
miles thick. The earth, though travel
ing with the velocity Of 1900, 600 miles a
day, is immersed in it for several days.
1.-THE fall Ut ,neteorites to the earth is
sometimes accompanied bya great dis
play of light, occasionally Illuminating
an area Of many thousand square miles
When such an event occurs at night, aud
with loud detonatons, 80 great in some
instances as to shake houses and fright
en- men and animals, the explosions are
caused by the breaking up Of the me-
teor. Ordinarily you will find that such
meteoric bodies are coated on the out
side with black substance, which is
the effect merely Of fusion of the super
fetal material by great heat. A piece Of
Biela's comet was actually picked up in
Mexico in 1879 at the time Of the shower
of it's remains. Naturally it is consid-
cred interesting. '~.-.. -
''Such great interest is taken in mete-
orites that all of those collected have
been carefully catalogued. They are
mostly composed Of iron, with usually .
percentage Of nickel and cobalt and
sometimes copper and tin. It is custom
ary to saw them into slices, which is
laborious process, for sale or for ex-
change among museums. Sometimes
the slices are prettily polished, or the cut
surfaces are etched with acid SO as to ex-
pose the crystalline structure. This
structure is in no two such bodies exact
" the same, and the differences are