Galilei, Galileo, The systems of the world, 1661

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SALV. You ſee then, that the Propoſition which ſaith, that
the
motion by the perpendicular is more ſwift than by the
nation
, holds not true univerſally, but onely of the motions,
which
begin from the extremity, namely from the point of reſt:
without
which reſtriction, the Propoſition would be ſo deficient,
that
its very direct contrary might be true; namely, that the
tion
in the inclining plane is ſwifter than in the perpendicular:
for
it is certain, that in the ſaid inclination, we may take a ſpace
paſt
by the moveable in leſs time, than the like ſpace paſt in the
perpendicular
.
Now becauſe the motion in the inclination is in
ſome
places more, in ſome leſs, than in the perpendicular;
fore
in ſome places of the inclination, the time of motion of the
moveable
, ſhall have a greater proportion to the time of the motion
of
the moveable, by ſome places of the perpendicular, than the
ſpace
paſſed, to the ſpace paſſed: and in other places, the
portion
of the time to the time, ſhall be leſs than that of the
ſpace
to the ſpace.
As for example: two moveables departing
from
their quieſcence, namely, from the point C, one by the
pendicular
C B, [in Fig. 4.] and the other by the inclination C A,
in
the time that, in the perpendicular, the moveable ſhall have
paſt
all C B, the other ſhall have paſt C T leſſer.
And therefore
the
time by C T, to the time by C B (which is equal) ſhall have
a
greater proportion than the line C T to C B, being that the
ſame to the leſs, hath a greater proportion than to the greater.
And
on the contrary, if in C A, prolonged as much as is
ſite
, one ſhould take a part equal to C B, but paſt in a ſhorter
time
; the time in the inclination ſhall have a leſs proportion to
the
time in the perpendicular, than the ſpace to the ſpace.
If
therefore
in the inclination and perpendicular, we may ſuppoſe
ſuch
ſpaces and velocities, that the proportion between the ſaid
ſpaces
be greater and leſs than the proportion of the times; we
may
eaſily grant, that there are alſo ſpaces, by which the times
of
the motions retain the ſame proportion as the ſpaces.

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