The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveries — John Shaqi
The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveriesGalilei, Galileo
History
The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveries
Galilei, Galileo
Astronomy -- Early works to 1800; Jupiter (Planet) -- Satellites
But here I feel that some people may be troubled with grave doubt, and
perhaps seized with a difficulty so serious as to compel them to feel
uncertain about the conclusion just explained and supported by so many
phenomena. For if that part of the Moon’s surface which reflects the
Sun’s rays most brightly is full of sinuosities, protuberances, and
cavities innumerable, why, when the Moon is increasing, does the outer
edge which looks toward the west, when the Moon is waning, the other
half-circumference towards the east, and at full-moon the whole circle,
appear not uneven, rugged, and irregular, but perfectly round and
circular, as sharply defined as if marked out with a pair of compasses,
and without the indentations of any protuberances or cavities? And most
remarkably so, because the whole unbroken edge belongs to that part of
the Moon’s surface which possesses the property of appearing brighter
than the rest, which I have said to be throughout full of protuberances
and cavities. For not one of the Great Spots extends quite to the
circumference, but all of them are seen to be together away from the
edge. Of this phenomenon, which affords a handle for such serious
doubt, I produce two causes, and so two solutions of the difficulty.
The first solution which I offer is this:—If the protuberances and
cavities in the body of the Moon existed only on the edge of the
circle that bounds the hemisphere which we see, then the Moon might,
or rather must, show itself to us with the appearance of a toothed
wheel, being bounded with an irregular and uneven circumference; but
if, instead of a single set of prominences arranged along the actual
circumference only, very many ranges of mountains with their cavities
and ruggednesses are set one behind the other along the extreme edge
of the Moon, and that too not only in the hemisphere which we see, but
also in that which is turned away from us, but still near the boundary
of the hemisphere, then the eye, viewing them afar off, will not at
all be able to detect the differences of prominences and cavities, for
the intervals between the mountains situated in the same circle, or in
the same chain, are hidden by the jutting forward of other prominences
situated in other ranges, and especially if the eye of the observer
is placed in the same line with the tops of the prominences mentioned.
So on the Earth, the summits of a number of mountains close together
appear situated in one plane, if the spectator is a long way off and
standing at the same elevation. So when the sea is rough, the tops of
the waves seem to form one plane, although between the billows there is
many a gulf and chasm, so deep that not only the hulls, but even the
bulwarks, masts, and sails of stately ships are hidden amongst them.
Therefore, as within the Moon, as well as round her circumference,
there is a manifold arrangement of prominences and cavities, and the
eye, regarding them from a great distance, is placed in nearly the
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