Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
=8. Meteors.= Everybody must, at some time, have beheld the phenomenon
known as a falling, or shooting, star. A few of these objects can be
seen darting across the sky on almost any clear night in the course of
an hour or two of watching. Sometimes they appear more numerously, and
at intervals they are seen in “showers.” They are called meteors, and it
is believed that they are minute solid bodies, perhaps averaging but a
small fraction of an ounce in weight, which plunge into the atmosphere
with velocities varying from twenty to thirty or more miles per second,
and are set afire and consumed by the heat of friction developed by
their rush through the air. Anybody who has seen a bullet melted by the
heat suddenly developed when it strikes a steel target has had a graphic
illustration of the transformation of motion into heat. But if we could
make the bullet move fast enough it would _melt in the air_, the heat
being developed by the constant friction.
The connection of meteors with comets is very interesting. In the year
1833, a magnificent and imposing display of meteors, which, for hours,
on the night between the 13th and 14th of November, filled the sky with
fire-balls and flaming streaks, astonished all beholders and filled many
with terror. It was found that these meteors travelled in an orbit
intersecting that of the earth at the point where the latter arrived in
the middle of November, and also that they had a period of revolution
about the sun of 33¼ years, and were so far scattered along their orbit
that they required nearly three years to pass the point of intersection
with the orbit of the earth. Thus it was concluded that for three years
in succession, in mid-November, there should be a display of the meteors
plunging into the earth's atmosphere. But only in the year when the
thickest part of the swarm was encountered by the earth would the
display be very imposing. Upon this it was predicted that there would be
a recurrence of the phenomenon of 1833 in the year 1866. It happened as
predicted, except that the number of meteors was not quite so great as
before. In the meantime, it had been discovered that these meteors
followed in the track of a comet known as Temple's Comet, and also that
certain other meteors, which appear every year in considerable numbers
about the 10th of August, followed the track of another comet called
Tuttle's Comet. Then in 1872 came the display, mentioned in the last
section, of meteors which were evidently the debris of the vanished
comet of Biela. The inference from so many similar cases was
irresistible that the meteors must be fragments of destroyed or
partially destroyed comets. Several other cases of identity of orbits
between meteors and comets have been discovered.
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