Galilei, Galileo, The systems of the world, 1661

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SAGR. The reſolutions, which between you two have been
alledged
touching this laſt doubt, hath, to ſpeak the truth,
ed
me alſo.
But at the ſame time this conſideration of the
fible
rayes accompanying the rayes of the Sun, hath begotten in me
another
ſcruple, about the other part, but I know not whether I
can
expreſſe it right, or no: for it but juſt now comming into my
mind
, I have not yet methodized it to my mind: but let us ſee if
we
can, all together, make it intelligible.
There is no queſtion,
but
that the parts towards the circumference of that poliſh't, but not
burniſh
't Hemiſphere, which is illuminated by the Sun, receiving the
rayes
obliquely, receive much fewer thereof, than the
moſt
parts, which receive them directly.
And its poſſible, that a
tract
or ſpace of v. g. twenty degrees in breadth, and which is
wards
the extremity of the Hemiſphere, may not receive more rays
than
another towards the middle parts, of but four degree broad:
ſo
that that doubtleſs will be much more obſcure than this; and
ſuch
it will appear to whoever ſhall behold them both in the face,
or
(as I may ſay) in their full magnitude.
But if the eye of the
beholder
were conſtituted in ſuch a place, that the breadth of the
twenty
degrees of the obſcure ſpace, appeared not to it longer
than
one of four degrees, placed in the midſt of the Hemiſphere,
I
hold it not impoſſible for it to appear to the ſaid beholder
qually
clear and lucid with the other; becauſe, finally, between
two
equal angles, to wit, of four degrees apiece, there come to
the
eye the reflections of two equal numbers of rayes: namely,
thoſe
which are reflected from the middlemoſt ſpace, four degrees
in
breadth, and thoſe reflected from the other of twenty degrees,
but
ſeen by compreſſion, under the quantity of four degrees: and
ſuch
a ſituation ſhall the eye obtain, when it is placed between the
ſaid
Hemiſphere, and the body which illuminates it; for then the
ſight
and rayes move in the ſame lines.
It ſeemeth not impoſſible
therefore
, but that the Moon may be of a very equal ſuperficies;
and
that nevertheleſſe, it may appear when it is at the full, no leſs

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