See next that which the obſervations of Peucerus giveth us, in
which the inferiour diſtance from the Pole is 28 gr. 21 m. and the
ſuperiour 28 gr. 2 m. the difference 0 gr. 19 m. and the diſtance
from the vertical point 66 gr. 27 m. from which particulars is
thered the ſtars diſtance from the centre almoſt 166
gr.m.AnglesI A C6627Sines91672I E C019553165 427/55355391672363973124which the inferiour diſtance from the Pole is 28 gr. 21 m. and the
ſuperiour 28 gr. 2 m. the difference 0 gr. 19 m. and the diſtance
from the vertical point 66 gr. 27 m. from which particulars is
thered the ſtars diſtance from the centre almoſt 166
Here take what Tycho his obſervation holdeth forth to us,
terpreted with greateſt favour to the adverſary; to wit, the
our diſtance from the pole is 28 gr. 13 m. and the ſuperiour 28 gr.
2 m. omitting the difference which is 0 gr. 11 m. as if all were one
Parallax; the diſtance from the vertical point 62 gr. 15 m. Behold
here below the operation, and the diſtance of the ſtar from the
centre found to be 976 9/16
gr.m.AnglesI A C6215Sines88500I E C011320276 9/163208850024181terpreted with greateſt favour to the adverſary; to wit, the
our diſtance from the pole is 28 gr. 13 m. and the ſuperiour 28 gr.
2 m. omitting the difference which is 0 gr. 11 m. as if all were one
Parallax; the diſtance from the vertical point 62 gr. 15 m. Behold
here below the operation, and the diſtance of the ſtar from the
centre found to be 976 9/16
The obſervation of Reinholdus, which is the next enſuing,
eth us the diſtance of the Star from the Centre 793.
eth us the diſtance of the Star from the Centre 793.
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