Appendix

Ml

East, the Meridian of any Place wi „■arrive at the Sun I in the Ecliptic, and a ^■wards at the Sun C in the Equinoctial >is, the Time of Noon by the Sun in d ie ^ c ],liptic will be sooner than that Noon f .,would happen by the Sun in the Equin° ^pand that by the Quantity of, the A sC ^turned into Time. -pit"

26. Now the Arch £ D = B C is & e ^ference of the Sun’s Longitude I os n tand his Right Ascension y B. Ag

parallel to D C, and the Angle j

equal to the Angle D S h, and thesimilar to the Arch D h ; therefore the ^in which the Meridian hf revolvesSituation ef is that which is to be $to the Ecliptic Noon to equate it ^

Time of the Equinoctial Noon in t ji£and third Quarters of the Ecliptic* ^second and fourth Quarter, the said ^tion is to be subtracted, as would eat 1pear by making the fame Const 1 * 1 'there, ^ of

27. Now because in different P al j sthe Quadrant this Arch D h or B 6 ^different Length, the Equation ofbe a variable Quantity; and therefn^ ^0the Motion and Time measured by * . jIn the Equinoctial is always equab