Salusbury, Thomas, Mathematical collections and translations (Tome I), 1667

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there
can be no obſervation of moment made, by reaſon it
fers
not it ſelf to be ſeen, ſave onely in its greateſt digrſſieons
from
the Sun, in which its diſtances from the earth are inſenſibly
unequal
, and thoſe differences conſequently not to be obſerved;
as
alſo its mutations of figures which muſt abſolutely happen in
it
, as in Venus. And if we do ſee it, it muſt of neceſſity appear
in
form of a Semicircle, as Venus likewiſe doth in her greateſt
digreſſions
; but its diſcus is ſo very ſmall, and its ſplendor ſo
very
great, by reaſon of its vicinity to the Sun, that the virtue
of
the Teleſcope doth not ſuffice to clip its treſſes or adventitious
rayes
, ſo as to make them appear ſhaved round about.
It

mains
, that we remove that which ſeemed a great inconvenience
in
the motion of the Earth, namely that all the Planets moving
about
the Sun, it alone, not ſolitary as the reſt, but in company
with
the Moon, and the whole Elementary Sphear, ſhould move
round
about the Sun in a year; and that the ſaid Moon withal
ſhould
move every moneth about the earth.
Here it is neceſſary
once
again to exclaim and extol the admirable perſpicacity of
pernicus
, and withal to condole his misfortune, in that he is not
now
alive in our dayes, when for removing of the ſeeming
ſurdity
of the Earth and Moons motion in conſort we ſee
ter
, as if it were another Earth, not in conſort with the Moon,
but
accompanied by four Moons to rovolve about the Sun in 12.
years
together, with what ever things the Orbs of the four
cæan
Stars can contain within them.

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