Harper's New Monthly Magazine, Vol. 3, July, 1851Various
History
Harper's New Monthly Magazine, Vol. 3, July, 1851
Various
American literature -- Periodicals; Civilization -- Periodicals; Culture -- Periodicals
Gold chain and seals, too! Well--it can't be helped. In these cases a
pinch of snuff often--often--pshaw!--often relieves--relieves
one--hillo! have I been relieved of that, also! Perhaps it's in my side
pocket, with my purse--purse! why, my purse is gone; I really begin to
think I must have been robbed!
CONCERNING THE ECLIPSES IN THE MONTH OF JULY, 1851.
BY CHARLES COLBY.
In the month of July, 1851, there will occur two eclipses; one of the
moon and one of the sun.
The former will occur after midnight, Sunday morning, July 13th; and the
latter on the morning of Monday, July 28th.
Unless clouds prevent, both will be visible throughout the United
States; and if visible will (the solar eclipse especially) attract
general observation.
[Illustration]
As here represented, there are formed complete shadows, called _umbras_;
and partial shadows, called _penumbras_.
When an eclipse of the sun occurs, it appears totally eclipsed to those
persons who are within the moon's umbra, and partially eclipsed, to
those situated within the penumbra.
When an eclipse of the moon occurs, it appears totally eclipsed, if
entirely within the earth's umbra, and partially eclipsed, if partially
within it.
The length of the moon's umbra is usually greater than the distance of
the moon from the earth.
[Illustration]
The moon, therefore, crosses the sun's path twice in each revolution.
If, at new moon, it always crossed exactly in that part where the sun
is, there would evidently be an eclipse of the sun; and it would recross
in the opposite part and pass through the earth's umbra.
But the moon does not always cross the ecliptic where the sun is, nor
uniformly in the same part.
Its crossing-place is different at each succeeding revolution.
[Illustration]
Since the limits of this article will not allow an extended explanation
of the manner of mathematically predicting eclipses, we will apply the
foregoing statements in showing that there will occur an eclipse of the
sun in July, 1851.
The first diagram on page 240 represents the relative positions of the
sun and moon at the time of new moon in June, July, and August, 1851,
calculated for Greenwich.
It is probable that there will be but few among the millions who may
thus behold these wonderful phenomena who will not understand their
causes.
However, an article explaining the manner of predicting these eclipses
with diagrams illustrating the path of the moon's shadow in the solar
eclipse across the United States and upon the whole earth, may not be
acceptable.
Since the earth and moon are solid opaque bodies, they intercept the
light passing from the sun through the heavens; or, in other words, they
cause the existence of shadows.
Hence, if the moon, in its revolution pass directly between the sun and
the earth its umbra will fall upon the earth, and cause a total eclipse
of the sun.
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