Galilei, Galileo
,
The systems of the world
,
1661
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think
of
accomodating
the
body
of
Venus
in
ſuch
a
manner
that
its
ſtate
and
motion
may
agree
with
what
ſenſible
experiments
do
ſhew
us
;
and
therefore
recall
to
mind
that
.
which
either
by
the
paſt
diſcourſes
,
or
your
own
obſervations
you
have
learnt
to
be
fal
that
ſtar
,
and
afterwards
aſſign
unto
it
that
ſtate
which
you
think
agreeth
with
the
ſame
.
SIMP.
Suppoſing
thoſe
Phænomena
expreſſed
by
you
,
and
which
I
have
likewiſe
read
in
the
little
treatiſe
of
Concluſions
,
to
[Figure 18]
be
true
,
namely
,
that
that
ſtar
never
recedes
from
the
Sun
beyond
ſuch
a
determinate
ſpace
of
40
degrees
or
thereabouts
,
ſo
as
that
it
never
cometh
either
to
appoſition
with
the
Sun
,
or
ſo
much
as
to
quadrature
,
or
yet
to
the
ſextile
aſpect
;
and
more
than
that
,
ſuppoſing
that
it
ſheweth
at
one
time
almoſt
40
times
greater
than
at
another
;
namely
,
very
great
,
when
being
retrograde
,
it
goeth
to
the
veſpertine
conjnnction
of
the
Sun
,
and
very
ſmall
when
with
a
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