[<emph type="italics"/>as in Fig.<emph.end type="italics"/> 5.] and the Axis, as before A C, by which the plane <lb/>
of our Meridian would pa&longs;&longs;e, in which plane &longs;hould al&longs;o be the <lb/>
Axis of the Suns revolution, with its Poles, one towards us, that <lb/>
is, in the apparent Hemi&longs;phere, which Pole we will repre&longs;ent by <lb/>
the point E, and the other &longs;hall fall in the occult Hemi&longs;phere, <lb/>
and I mark it I. </s><s>Inclining therefore the Axis E I, with the &longs;upe <lb/>
riour part E, towards us, the great circle de&longs;cribed by the Suns <lb/>
conver&longs;ion, &longs;hall be this B F D G, who&longs;e half by us &longs;een, name <lb/>
ly B F D, &longs;hall no longer &longs;eem unto us a right line, by rea&longs;on the <lb/>
Poles E I are not in the circumference A B C D, but &longs;hall appear <lb/>
incurvated, and with its convexity towards the inferiour part C. <lb/>
</s><s>And it is manife&longs;t, that the &longs;ame will appear in all the le&longs;&longs;er cir <lb/>
cles parallel to the &longs;ame B F D. </s><s>It is to be under&longs;tood al&longs;o, that <lb/>
when the Earth &longs;hall be diametrically oppo&longs;ite to this &longs;tate, &longs;o <lb/>
that it &longs;eeth the other Hemi&longs;phere of the Sun, which now is hid, <lb/>
it &longs;hall of the &longs;aid great circle behold the part D G B incurved, <lb/>
with its convexity towards the &longs;uperiour part A; and the cour <lb/>
&longs;es of the &longs;pots in the&longs;e con&longs;titutions &longs;hall be fir&longs;t, by the arch <lb/>
B F D, and afterwards by the other D G B, and the fir&longs;t appari <lb/>
tions and ultimate occultations made about the points B and D, <lb/>
&longs;hall be equilibrated, and not tho&longs;e that are more or le&longs;&longs;e eleva <lb/>
ted than the&longs;e. </s><s>But if we con&longs;titute the Earth in &longs;uch a place <lb/>
of the Ecliptick, that neither the boundary A B C D, nor the <lb/>
Meridian A C, pa&longs;&longs;eth by the Poles of the Axis E I, as I will &longs;hew <lb/>
you anon, drawing this other Figure [<emph type="italics"/>viz. </s><s>Fig.<emph.end type="italics"/> 6.] wherein the <lb/>
apparent or vi&longs;ible Pole E falleth between the arch of the termi <lb/>
nator A B, and the &longs;ection of the Meridian A C; the diameter <lb/>
of the great circle &longs;hall be F O G, and the apparent &longs;emicircle <lb/>
F N G, and the occult &longs;emicircle G S F, the one incurvated with <lb/>
its convexity N towards the inferiour part, and the other al&longs;o <lb/>
bending with its convexity S towards the upper part of the Sun. <lb/>
</s><s>The ingre&longs;&longs;ions and exitions of the &longs;pots, that is, the termes F <lb/>
and G &longs;hall not be librated, as the two others B and D; but F <lb/>
&longs;hall be lower, and G higher: but yet with le&longs;&longs;er difference <lb/>
than in the fir&longs;t Figure. </s><s>The arch al&longs;o F N G &longs;hall be incurva <lb/>
ted, but not &longs;o much as the precedent B F D; &longs;o that in this po <lb/>
&longs;ition the pa&longs;&longs;ages or motions of the &longs;pots &longs;hall be a&longs;cendent <lb/>
from the left &longs;ide F, towards the right G, and &longs;hall be made by <lb/>
curved lines. </s><s>And imagining the Earth to be con&longs;tituted in the <lb/>
po&longs;ition diametrically oppo&longs;ite; &longs;o that the Hemi&longs;phere of the <lb/>
Sun, which was before the occult, may be the apparent, and ter <lb/>
minated by the &longs;ame boundary A B C D, it will be manife&longs;tly <lb/>
di&longs;cerned, that the cour&longs;e of the &longs;pots &longs;hall be by the arch G S F, <lb/>
beginning from the upper point G, which &longs;hall then be likewi&longs;e <lb/>
from the left hand of the beholder, and going to determine, de&longs;