Galilei, Galileo, The systems of the world, 1661

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SAGR. I clearly perceive all this, and underſtand very well,
that
the Moon departing from its Oppoſition to the Sun, where it
ſaw
no part of the illumination of the Terreſtrial ſuperficies, and
approaching
day by day nearer the Sun, ſhe begins by little and
little
to diſcover ſome part of the face of the illuminated Earth;
and
that which appeareth of it ſhall reſemble a thin ſickle, in regard
the
figure of the Earth is round: and the Moon thus acquiring by
its
motion day by day greater proximity to the Sun, ſucceſſively
diſcovers
more and more of the Terreſtrial Hemiſphere enlightned,
ſo
that at the Quadrature there is juſt half of it viſible, inſomuch
that
we may ſee the other part of her: continuing next to proceed
towards
the Conjunction, it ſucceſſively diſcovers more and more
of
its ſurface to be illuminated, and in fine, at the time of
ction
ſeeth the whole Hemiſphere enlightned.
And in ſhort, I
very
well conceive, that what befalls the Inhabitants of the Earth,
in
beholding the changes of the Moon, would happen to him that
from
the Moon ſhould obſerve the Earth; but in a contrary order,
namely
, that when the Moon is to us at her full, and in Oppoſition
to
the Sun, then the Earth would be in Conjunction with the Sun,
and
wholly obſcure and inviſible; on the contrary, that poſition
which
is to us a Conjunction of the Moon with the Sun, and for
that
cauſe a Moon ſilent and unſeen, would be there an Oppoſition
of
the Earth to the Sun, and, to ſo ſpeak, Full Earth, to wit, all
enlightned
.
And laſtly, look what part of the Lunar ſurface
pears
to us from time to time illuminated, ſo much of the Earth
in
the ſame time ſhall you behold from the Moon to be obſcured:
and
look how much of the Moon is to us deprived of light, ſo much
of
the Earth is to the Moon illuminated.
In one thing yet theſe
mutual
operations in my judgment ſeem to differ, and it is, that it

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