Appendix.

Neatest of all; arid from this Time

^0 ^ “ UU1 <■“*=> J. uut it

^ VVs less t;u the Sun arrives at the 90th^of ee ’ Solstice) when the Line of

j , es are in the Quadratures, and then itle *st of all.

Therefore twice in a Year the In-Ration of the Ecliptic and Equator ist^‘ fished) and twice again restored ; and(X Hodes (or Equinoxes) constantly go4 ^ War ds, and carry the Axis of the Eartha . ^ith a retrograde Motion about thePj ts of the Ecliptic T F, tracing out theK* 2 ° r ratlner vermicular Curve HIGHo Heavens among the Fixed Stars,is ?°* ; the Plane of the Equator

^ lric iin e d to the Plane of the Moon’s Or-for the latter makes an Angle of but5 Degrees with the Plane of the^ j HC; anc } therefore the Moon (thoughf) r ^ s Sody than the Sun, yet being nearer)tjj Uc es a greater Effect than the Sun on^ctuatorial Ring or Zone of Matter,f° augments all the aforesaid MotionsEarth’s Plane and Axis. Sir Isaac\\ t0H ^ as Xewn fProp . XXXIX. Lib. III.)tke Part of the annual Recestion of the)°xes, which is owing to the Sun, is

owing to

Th5 N'',

Ikl 2o A and that'which is

°°tt is 40" 52 " $A a

^ ^ “o''"

therefore by thejoint

355