Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
Since an inferior planet circulates between us and the sun, one would be
inclined to expect that such a body, each time it passed on the side
nearest to the earth, should be seen as a black spot against the bright
solar disc. Now this would most certainly be the case were the orbit of
an inferior planet in the same plane with the orbit of the earth. But we
have already seen how the orbits in the solar system, whether those of
planets or of satellites, are by no means in the one plane; and that it
is for this very reason that the moon is able to pass time after time in
the direction of the sun, at the epoch known as new moon, and yet not to
eclipse him save after the lapse of several such passages. Transits,
then, as the passages of an inferior planet across the sun's disc are
called, take place, for the same reason, only after certain regular
lapses of time; and, as regards the circumstances of their occurrence,
are on a par with eclipses of the sun. The latter, however, happen much
more frequently, because the moon passes in the neighbourhood of the
sun, roughly speaking, once a month, whereas Venus comes to each
inferior conjunction at intervals so long apart as a year and a half,
and Mercury only about every four months. From this it will be further
gathered that transits of Mercury take place much oftener than transits
of Venus.
Until recent years _Transits of Venus_ were phenomena of great
importance to astronomers, for they furnished the best means then
available of calculating the distance of the sun from the earth. This
was arrived at through comparing the amount of apparent displacement in
the planet's path across the solar disc, when the transit was observed
from widely separated stations on the earth's surface. The last transit
of Venus took place in 1882, and there will not be another until the
year 2004.
_Transits of Mercury_, on the other hand, are not of much scientific
importance. They are of no interest as a popular spectacle; for the
dimensions of the planet are so small, that it can be seen only with the
aid of a telescope when it is in the act of crossing the sun's disc. The
last transit of Mercury took place on November 14, 1907, and there will
be another on November 6, 1914.
The first person known to have observed a transit of an inferior planet
was the celebrated French philosopher, Gassendi. This was the transit of
Mercury which took place on the 7th of December 1631.
Public-domain text, read in full here on John Shaqi.
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