Ptolemy's Tetrabiblos : $b or Quadripartite, being four books of the influence of the stars ... with a preface, explanatory notes, and an appendix containing extracts from the Almagest of Ptolemy and the whole of his Centiloquy, together with a short notice of Mr. Ranger's zodiacal planisphere and an explanatory platePtolemy
Religion
Ptolemy's Tetrabiblos : $b or Quadripartite, being four books of the influence of the stars ... with a preface, explanatory notes, and an appendix containing extracts from the Almagest of Ptolemy and the whole of his Centiloquy, together with a short notice of Mr. Ranger's zodiacal planisphere and an explanatory plate
Ptolemy
Astrology -- Early works to 1800
When it has been ascertained what degree of the zodiac is on the
mid-heaven, as also which are the preceding and succeeding degrees,
the period of whose meeting is to be calculated, the position of the
preceding degree, and its distance in temporal hours from the meridian,
are next to be noted; because any part of the zodiac, on becoming
distant from the meridian in the same temporal hours, must fall on the
same individual semicircle.[164] For ascertaining this distance, the
number of ascensions, in a right sphere, found in the intermediate
space between the said preceding degree and the mid-heaven, either
above or under the earth, is to be divided by the number of the diurnal
or nocturnal horary times of the said preceding degree: for instance,
if that degree be above the earth, by its diurnal horary times; and, by
its nocturnal, if it be under the earth. It is then to be discovered in
what number of equatorial times the succeeding degree will be distant
from the same meridian, by as many similar temporal hours as those by
which the preceding degree is distant from it. And, to effect this,
the hours in question must be noted, and it must first be observed, by
the right ascensions again, how many equatorial times the succeeding
degree, at its original position, is distant from the degree on the
mid-heaven; and then it must be seen how many equatorial times it will
be distant, on coming to the preceding degree’s distance in temporal
hours from the said mid-heaven: this will be found, by multiplying
those hours by the succeeding degree’s horary times; diurnal, if the
future position be above the earth, and nocturnal if under; and the
difference in amount, of these two distances, in equatorial times, will
present the number of years inquired for.
[164] _Vide_ Note ², p. 95.
CHAPTER XV
EXEMPLIFICATION
In order to exemplify the foregoing instructions, let the first point
of Aries be supposed as the preceding place, and the first point in
Gemini the succeeding; and let the latitude of the country, to which
the operation relates, be such as will cause the longest day to consist
of fourteen hours[165]; and where the horary magnitude of the beginning
of Gemini will be about seventeen equatorial times.[166]
[165] This, in the Northern Hemisphere, would be the latitude of
Alexandria (where Ptolemy flourished), or, in his own words, that of
the 3rd Climate, passing through Lower Egypt, numbered 30° 22′.—_Vide_
extracts from the Tables of the Almagest, inserted in the Appendix.
[166] This is the magnitude of the diurnal temporal hour of the first
point of Gemini in the latitude prescribed.
Public-domain text, read in full here on John Shaqi.
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