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
In observations to determine the exact positions of celestial objects
correction has to be made for the effects of refraction, according to
the apparent elevation of these objects in the sky. Such effects are
least when the objects in question are directly overhead, for then the
rays of light, coming from them to the eye, enter the atmosphere
perpendicularly, and not at any slant.
A very curious effect, due to refraction, has occasionally been observed
during a total eclipse of the moon. To produce an eclipse of this kind,
_the earth must, of course, lie directly between the sun and the moon_.
Therefore, when we see the shadow creeping over the moon's surface, the
sun should actually be well below the horizon. But when a lunar eclipse
happens to come on just about sunset, the sun, although really sunk
below the horizon, appears still above it through refraction, and the
eclipsed moon, situated, of course, exactly opposite to it in the sky,
is also lifted up above the horizon by the same cause. Pliny, writing in
the first century of the Christian era, describes an eclipse of this
kind, and refers to it as a "prodigy." The phenomenon is known as a
"horizontal eclipse." It was, no doubt, partly owing to it that the
ancients took so long to decide that an eclipse of the moon was really
caused by the shadow cast by the earth. Plutarch, indeed, remarks that
it was easy enough to understand that a solar eclipse was caused by the
interposition of the moon, but that one could not imagine by the
interposition _of what body_ the moon itself could be eclipsed.
In that apparent movement of the heavens about the earth, which men now
know to be caused by the mere rotation of the earth itself, a slight
change is observed to be continually taking place. The stars, indeed,
are always found to be gradually drawing westward, _i.e._ towards the
sun, and losing themselves one after the other in the blaze of his
light, only to reappear, however, on the other side of him after a
certain lapse of time. This is equivalent to saying that the sun itself
seems always creeping slowly _eastward_ in the heaven. The rate at which
this appears to take place is such that the sun finds itself back again
to its original position, with regard to the starry background, at the
end of a year's time. In other words, the sun seems to make a complete
tour of the heavens in the course of a year. Here, however, we have
another illusion, just as the daily movement of the sky around the earth
was an illusion. The truth indeed is, that this apparent movement of the
sun eastward among the stars during a year, arises merely from a
_continuous displacement of his position_ caused by an actual motion of
the earth itself around him in that very time. In a word, it is the
earth which really moves around the sun, and not the sun around the
earth.
Public-domain text, read in full here on John Shaqi.
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