The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
having fallen during a long period, that a slight preponderance in
respect of quantity falls near the ‘new’ Moon over that which falls near
the ‘full.’ This would be a natural and necessary consequence of a
preponderance of a cloudless sky about the ‘full,’ and forms, therefore,
part and parcel of the same meteorological fact.”
Bernadin has asserted it to be a fact that many thunderstorms occur
about the period of “new” or “full” Moon. But what I want most to warn
the reader against is that popular idea (wonderfully wide-spread it must
be admitted) that at the epochs of what are called, most illogically,
the Moon’s “changes,” changes of weather may certainly be expected.
There is absolutely no foundation whatever for this, and still more void
of authority (if such a phrase is admissible) is a table of imaginary
weather to be expected at changes of the Moon, often met with in books
published half a century ago, and still occasionally reprinted in
third-rate almanacs, and designated “Dr. Herschel’s Weather Table.” This
precious production is not only devoid of authenticity as regards its
name, but may easily be seen to be fraudulent in its reputed facts any
month in the year.
It would be beyond both my present available space and the legitimate
objects of this work to attempt even an outline of the influences over
things terrestrial ascribed to, or associated, rightly or wrongly, with
the Moon, and of which the word “lunatic” perhaps affords the most
familiar exponent.
CHAPTER VII.
MARS.
Mars, though considerably smaller than the Earth, is commonly regarded
as the planet which, taken all in all, bears most resemblance to the
Earth, though only one-fourth its size. Under circumstances which have
already been briefly alluded to in Chapter I., Mars exhibits from time
to time a slight phase, but nothing approaching in amount the phases
presented by the two inferior planets, Mercury and Venus. When in
opposition to the Sun, that is to say when on the meridian at midnight,
it has a truly circular disc; but between opposition and its two
positions of quadrature it is gibbous. At the minimum phase, which is at
each quadrature, E. or W. as the case may be, the planet resembles the
Moon 3 days from its “full.” These phases are an indication that Mars
shines by the reflected light of the Sun. It is a remarkable tribute to
Galileo’s powers of observation that with his trumpery telescope, only a
few inches long, he should have been able to suspect the existence of a
Martial phase. Writing to a friend in 1610 he says:—“I dare not affirm
that I can observe the phases of Mars; however, if I mistake not, I
think I already perceive that he is not perfectly round.”
[Illustration: Fig. 12.—Four views of Mars differing 90° in longitude
(Barnard).]
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