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卷二十一 志第二: 曆上 步氣朔第一 步卦候第二 步日躔第三

Volume 21 Treatises 2: Calendar 1 - Seasonal Phases and Month Beginnings 1, Phases and Divination 2, Phases of the Sun's Path 3

Chapter 21 of 金史 · History of Jin
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1
退
Long ago the sages took Heaven's Way to give mankind the seasons, set the hundred offices in order to brighten common affairs—and the arts of stepwise reckoning reach back to a remote antiquity. From the Han Taichu era down to the former Song, calendar-makers numbered more than seventy houses; as a rule, every century or few decades brought a new system. Sun, moon, and five stars swell and shrink, advance and retreat; Heaven's motion is never uniform. Men fashion reckonings to force alignment—but piling small errors into large ones, some discrepancy is inevitable.
2
Jin held the realm for a little over a century and changed its calendar only once. In Tianhui year 5 the Director of Heaven Yang Ji completed the Grand Clarity Calendar; in spring of year 15, on the new moon of the first month, it was first promulgated. Its constants take 383,768,657 as the calendar origin and 5,230 as the day divisor. Its sources cannot be traced in full; some say it was adapted from the Song Era Origin Calendar with additions and cuts. Zhenglong, wuyin year, third month, on xinyou, the new moon: the calendar office predicted an eclipse, but none occurred. Dading guisi, fifth month, on renchen, the new moon—a solar eclipse; jiawu, eleventh month, on jiashen, the new moon—another eclipse; in both cases the predicted time came before the event. Dingyou, ninth month, on dingyou, the new moon—the eclipse came after the predicted hour. Prognostication and observation drifted apart; the Directorate ordered Zhao Zhiwei to revise the Grand Clarity Calendar, and in eleven years the revision was done. At the same time Hanlin Attendant Yelü Lü also devised the Yiwei Calendar. In year 21, at the full moon of the eleventh month, the moon was eclipsed; the Ministry ordered Ren Zhongjie of the Rites Bureau and the calendar officers to verify the hour, minute, and second of the eclipse and compare Zhao Zhiwei's, Yelü Lü's, and the current calendar—Zhiwei's proved closer, and his calendar was adopted. Early in Mingchang the calendar office proposed yet another revision; Zhang Xingjian of the Rites Bureau said, "Wait for another solar eclipse, re-check until there is no discrepancy, and only then adopt it." The proposal was shelved. Through the whole Jin age only Zhao Zhiwei's calendar was used; our dynasty used it at first as well, then replaced it with the Season-Granting Calendar. Its text still rests with the Grand Astrologer; we have gathered and recorded it here as the Calendar Treatise.
3
Procedures for qi and new moon, part one.
4
Era computation: from upper origin jiazi to the present Dading gengzi, 88,639,656 years.
5
Day divisor: 5,230 parts.
6
Tropical year dividend: 1,910,224 parts.
7
Common remainder: 27,424 parts.
8
New-moon dividend: 154,445 parts.
9
Common intercalation: 56,884 parts.
10
Year stride: 365 days, remainder 1,274 parts.
11
New-moon stride: 29 days, remainder 2,775 parts.
12
Qi stride: 15 days, remainder 1,142 parts, 60 seconds.
13
Full-moon stride: 14 days, remainder 4,002 parts, 45 seconds.
14
Phase stride: 7 days, remainder 2,001 parts, 22 and a half seconds.
15
Submergence limit: 4,087 parts, 30 seconds.
16
New-moon void fraction: 2,455 parts.
17
Ten-day circuit: 313,800 parts.
18
Era divisor: 60.
19
Second parent: 90.
20
To find the winter solstice of the celestial standard year.
21
滿
Set the accumulated years since upper origin jiazi, multiply by the tropical year dividend to obtain the general accumulated parts. Cast out full ten-day circuits; divide the remainder by the day divisor for days, with the unfilled portion as the remainder; count outside jiazi—that yields the greater and lesser remainders for the celestial-standard winter solstice.
22
To find successive qi.
23
滿
Set the winter solstice greater and lesser remainders and add the qi stride cumulatively; when seconds fill the second parent they carry into parts, when parts fill the day divisor they carry into days—thus each successive qi day with its remainder and seconds.
24
To find the canonical new moon of the celestial standard year.
25
滿
Divide the general accumulated parts by the new-moon dividend; the remainder is the intercalary remainder; subtract it from the general accumulated parts to obtain the new-moon accumulated parts. Cast out full ten-day circuits; divide the remainder by the day divisor for days, with the unfilled portion as the remainder—that yields the greater and lesser remainders for the celestial-standard canonical new moon.
26
To find quarter-moon, full-moon, and successive new moons.
27
Set the canonical new moon greater and lesser remainders and add the phase stride cumulatively—each addition yields the quarter-moon, full-moon, and successive canonical days with their remainders and seconds.
28
To find submergence days.
29
滿
Take the lesser remainder of the constant qi that bears submergence; if it reaches the submergence limit or above, that qi has a submergence day. Multiply by the second parent and include the seconds; subtract from 477,556; divide the remainder by 6,856 and add to the constant qi greater remainder—name the result as the submergence day.
30
To find extinction days.
31
滿
Take the lesser remainder of the new moon that bears extinction—when the canonical new moon lesser remainder falls short of the new-moon void fraction. Multiply by six, divide by 491, add to the canonical new moon greater remainder—name the result as the extinction day.
32
Procedure 2: Hexagrams and Period-Markers.
33
Hou rule: 5 days, remainder 380 parts, 80 seconds.
34
Hexagram rule: 6 days, remainder 457 parts, 6 seconds.
35
Zhen rule: 3 days, remainder 228 parts, 46 seconds.
36
Second denominator: 90.
37
Chen divisor: 2,615.
38
Half-chen divisor: 1,307½.
39
Ke divisor: 313 parts, 80 seconds.
40
Chen-ke: 8 parts, 104 fen, 60 seconds.
41
Half-chen ke: 4 parts, 52 fen, 30 seconds.
42
Second denominator: 100.
43
To find the seventy-two hou.
44
Take the mid-qi major and minor remainders as the first hou; by cumulative addition of the hou rule you reach each subsequent hou and the final hou.
45
To find the sixty-four hexagrams.
46
Take the mid-qi major and minor remainders and designate them as the duke hexagram; by cumulative addition of the hexagram rule you obtain the lord hexagram; add again to obtain the marquis inner hexagram. add the zhen rule to reach the start of the qi-period, the marquis outer hexagram; add the zhen rule again to obtain the grandee hexagram. add the hexagram rule again for the minister hexagram.
47
To find the Earth ruler's dominion.
48
Subtract the zhen rule from each season's mid-qi major and minor remainders to obtain the Earth ruler's dominion day.
49
To find expansion and contraction.
50
Set the minor remainder, multiply by six, and divide by the chen divisor to obtain the chen number. If any remainder remains, divide it by the ke divisor to obtain ke. Count outward from zi below the stem sequence to obtain the double-hour, ke, and fen of the added time. If the half-chen divisor is included, count from the beginning of the zi ke.
51
Procedure 3: Solar Motion along the Ecliptic.
52
Circuit-of-heaven parts: 1,910,293 parts, 530 seconds.
53
Precession: 69 parts, 530 seconds. Second denominator: 10,000.
54
Calibrated circuit of heaven: 365° 25′ 68″.
55
Quadrant limit: 91° 31′ 9″.
56
Daily accumulated degrees and excess–deficit for the twenty-four qi-periods.
57
To find the daily excess–deficit and tuoke.
58
Set each qi-period's gain-and-loss rate to derive excess–deficit gain and loss, and use the tuoke gain-and-loss rate for tuoke. Multiply by six and divide by the quadrant limit to obtain the mid-qi rate. Subtract from the next qi-period's mid-qi rate to obtain the combined difference. Add or subtract half the combined difference from the mid-qi rate to obtain the initial and final general rates. After a solstice: add to the initial, subtract from the final. After an equinox: subtract from the initial, add to the final. Set the combined difference, multiply by six, divide by the quadrant limit for days; halve and add or subtract from the initial and final general rates to obtain the initial and final fixed rates. After a solstice: subtract from the initial, add to the final. After an equinox: add to the initial, subtract from the final. By cumulative daily difference add and subtract the qi-period's initial and final fixed rates to obtain the daily gain-and-loss parts. After a solstice subtract; after an equinox add. Apply each day's gain-and-loss parts to adjust the qi-period's excess–deficit and tuoke accumulations for the daily values; whenever the combined difference derives from subtracting the preceding qi's original and following rates, use that preceding qi's combined difference.
59
To find qi entry for major new moon, first quarter, full moon, and last quarter.
60
滿 滿
Set the Heavenly Origin intercalary remainder; divide by the day divisor for days and keep the remainder; if below the qi rule, subtract from the qi rule to obtain entry into Major Snow. Remove what is above; subtract the qi rule from the remainder again to obtain entry into Minor Snow. This yields the day and remainder of the civil new year’s mean conjunction within its qi phase. Add the image strategy repeatedly; discard a full qi strategy each time to obtain the day and remainder within the next qi for first quarter and full moon. Continue adding likewise to obtain each later conjunction’s day and remainder within its qi phase.
61
Procedure to find each day’s deficit and surplus, expansion and contraction, and deficit–surfeit.
62
Apply the daily difference to add or subtract the initial qi-phase deficit–surplus rate and obtain the daily deficit–surplus rate. Accumulate stepwise to adjust the qi-phase expansion–contraction and deficit–surfeit totals into the daily expansion and deficit–surfeit accumulations.
63
Procedure to find the fixed deficit–surfeit number for mean conjunction and waxing and full moon within qi.
64
Multiply the entered constant qi’s minor remainder by the daily deficit–surplus rate, divide by the day divisor, and apply the result to the underlying deficit–surfeit accumulation to obtain the fixed number.
65
宿
Equatorial lodge degrees.
66
Dipper 25°; Ox 7° minor; Maid 11° minor; Void 9° minor, 68″; Rooftop 15° half; Encampment 17°; Wall 8° major.
67
宿
At right: the northern seven lodges total 94° 68″.
68
Striding Man 16° half; Bond 12°; Stomach 15°; Hairy Head 11° minor; Net 17° minor; Beak 0.5°; Three Stars 10° half.
69
西宿
At right: the western seven lodges 83°; Well 33° minor; Ghost 2° half; Willow 13° major; Star 6° major; Extended Net 17° minor; Wings 18° major; Chariot Axis 17°.
70
宿
At right: the southern seven lodges 109° minor; Horn 12°; Gullet 9° minor; Base 16°; Chamber 5° major; Heart 6° minor; Tail 19° minor; Winnowing Basket 10° half.
71
宿
At right: the eastern seven lodges total 79°.
72
Procedure to find the winter solstice equatorial solar degree.
73
滿退 宿滿宿
Set the general accumulated parts, subtract the circuit-of-heaven parts, divide the remainder by the day divisor for degrees, and convert the remainder into minutes and seconds. Use one hundred as the denominator. Count from beyond Void lodge 7° on the equator and discard full lodges; the lodge not yet filled gives the winter solstice hour-of-addition equatorial solar degree and minutes and seconds for the civil new year of the year sought.
74
Procedure to find the equatorial solar degrees at spring equinox, summer solstice, and autumn equinox.
75
滿宿宿
Set the winter solstice equatorial degree at hour-of-addition, add the image quadrant repeatedly, and discard full equatorial cycles to obtain the equatorial lodge degrees and minutes and seconds at hour-of-addition for spring equinox, summer solstice, and autumn equinox.
76
宿
Procedure to find the accumulated equatorial degrees after the four cardinals.
77
宿 宿宿
Set the full width of each cardinal equatorial lodge, subtract the cardinal equatorial solar degree and minutes, and the remainder is the post-cardinal distance. Add equatorial lodge widths cumulatively to obtain the accumulated equatorial degree and minutes after each cardinal.
78
宿
Procedure to find whether an equatorial accumulated degree falls in the initial or terminal limit.
79
宿
If the post-cardinal equatorial accumulation is 45° 65′ 54.5″ or less, it is in the initial limit; otherwise subtract it from the image quadrant and the remainder is in the terminal limit.
80
宿
Procedure to find the ecliptic degrees of the twenty-eight lodges.
81
宿滿滿 宿宿 宿宿宿 宿
Subtract the post-cardinal equatorial limit from 101°, multiply by the limit’s degrees and minutes, carry as needed, and convert hundreds into minutes and then into degrees. Subtract after winter solstice and add after the equinoxes to convert equatorial accumulation into ecliptic accumulation for each lodge. Subtract the prior lodge’s ecliptic accumulation; for the four cardinal lodges, add the image quadrant first, then subtract the prior lodge. The result is that lodge’s ecliptic degree and minutes. Round the minutes to major, half, and minor fractions.
82
宿
Ecliptic lodge degrees.
83
Dipper 23°; Ox 7°; Maid 11°; Void 9° minor, 68″; Rooftop 16°; Encampment 18° minor; Wall 9° half.
84
宿
At right: the northern seven lodges total 94° 68″.
85
Striding Man 17° major; Bond 12° major; Stomach 15° half; Hairy Head 11°; Net 16° half; Beak 0.5°; Three Stars 9° major.
86
西宿
At right: the western seven lodges 83° major; cumulative 177°, 75′, 68″.
87
Well 30° half; Ghost 2° half; Willow 13° minor; Star 6° major; Extended Net 17° major; Wings 20°; Chariot Axis 18° half.
88
宿
At right: the southern seven lodges 109° minor; cumulative 287°, 68″.
89
Horn 12° major; Gullet 9° major; Base 16° minor; Chamber 5° major; Heart 6°; Tail 18° minor; Winnowing Basket 9° half.
90
宿
At right: the eastern seven lodges 78° minor; cumulative 365°, 25′, 68″.
91
宿 宿
The ecliptic lodge degrees above are determined by the present calendar’s precessional position. To check the past and test the future, rely on precession: whenever it shifts a degree, recalculate contemporary lodge degrees by the procedure—only then can the seven luminaries be stepped and their places known.
92
Procedure to find the ecliptic solar degree at civil new-year winter solstice hour-of-addition.
93
滿滿
Subtract 101° from the winter solstice equatorial degree at hour-of-addition, multiply the remainder by that equatorial degree and its minutes and seconds, carry, and convert hundreds into minutes and then degrees. This is called the ecliptic–equator difference. Subtract that difference from the winter solstice equatorial degree at hour-of-addition to obtain the ecliptic solar degree and minutes and seconds at civil new-year winter solstice for the year sought.
94
Procedure to find the ecliptic solar degrees at hour-of-addition for all twenty-four qi.
95
宿宿 宿宿
Take the winter solstice ecliptic–equator difference for the year sought, subtract the next year’s difference, multiply the remainder by the qi number and divide by twenty-four, add to the qi’s central accumulation and approximate parts, adjust by the first-day expansion–contraction (surplus add, contraction subtract), add to the winter solstice ecliptic degree at hour-of-addition, and discard full lodge cycles to obtain each qi’s ecliptic solar lodge at hour-of-addition. If the winter solstice equatorial lodge at hour-of-addition has fractional minutes and seconds below the precessional threshold, add the prior lodge’s full width before computing the ecliptic–equator difference; otherwise follow the procedure as above.
96
To find the daily ecliptic solar degree before dawn and at midnight for each of the twenty-four qi.
97
滿退
Set aside the qi's minor remainder, multiply by that qi's first-day decrease-increase rate, and apply excess-and-deficit to the decrease and increase. Reduce by ten thousand to obtain fen; for increase, excess-add and deficit-subtract; for decrease, excess-subtract and deficit-add the subsidiary; divide by the day factor for degrees, and any remainder steps back into fen and miao; subtract from that qi's added-hour ecliptic solar degree to obtain each qi's first-day ecliptic solar degree before dawn and at midnight. Add one degree each day, reduce the daily decrease-increase rate by one hundred, and apply excess-and-deficit to the decrease and increase. For increase, excess-add and deficit-subtract; for decrease, excess-subtract and deficit-add — yielding the daily ecliptic solar degree before dawn and at midnight with fen and miao.
98
To find the daily noon ecliptic solar degree.
99
滿滿宿
Set ten thousand fen, take the entered qi's daily excess-deficit decrease-increase rate, and for increase excess-add and deficit-subtract, for decrease excess-subtract and deficit-add; add and subtract the decrease-increase rate throughout, halve the remainder, convert hundreds to fen and the remainder to miao, and add to that day's early-morning before-dawn ecliptic solar degree to obtain the noon solar progression ecliptic lodge degree with fen and miao.
100
To find the daily noon accumulated ecliptic degree.
101
From the solstice added-hour ecliptic solar degree, measure to the sought day's noon ecliptic solar degree to obtain the accumulated ecliptic degree after the solstice, with fen and miao.
102
Daily noon ecliptic entry into initial and final limits.
103
滿
For accumulated ecliptic degree after a solstice: at 43°12′87″ or below, it is the initial limit; above that, subtract the quadrant limit and the remainder is entry into the final limit. When the accumulated degree fills the quadrant limit, remove it to obtain the post-equinox accumulated ecliptic degree; at 48°18′22″ or below it is the initial limit; above that, subtract the quadrant limit and the remainder is entry into the final limit.
104
To find the daily noon equatorial solar degree.
105
Take the sought day's noon accumulated ecliptic degree — after a solstice in the initial limit, after an equinox in the final limit — with degrees, fen, and miao; advance three places, add 202,050 and a fraction less, take the square root and divide; subtract 449.5; if in the initial limit, add the two-solstice equatorial solar degree directly and assign the mansions. If in the final limit, subtract the quadrant limit, add the two-equinox equatorial solar degree to the remainder, and assign the mansions. That yields the daily noon equatorial solar degree. Take the sought day's noon accumulated ecliptic degree — after a solstice in the final limit, after an equinox in the initial limit — with degrees, fen, and miao; advance three places, subtract 303,050 and a fraction less, take the square root and divide; subtract 550.5; if in the initial limit, add the two-equinox equatorial solar degree to the remainder and assign the mansions. If in the final limit, subtract the quadrant limit, add the two-solstice equatorial solar degree to the remainder, and assign the mansions. That yields the daily noon equatorial solar degree.
106
宿 滿
Solar ecliptic twelve-lodge palace-entry degrees: Rain Water — beyond 13°39′50″ of Wei, enters the Wei allotment, Zouzi station, sign at hai. Spring Equinox — beyond 2°35′85″ of Kui, enters the Lu allotment, Jianglou station, sign at xu. Grain Rain — beyond 4°24′33″ of Stomach, enters the Zhao allotment, Daliang station, sign at you. Lesser Fullness — beyond 7°96′6″ of Net, enters the Jin allotment, Shishen station, sign at shen. Summer Solstice — beyond 9°47′10″ of Well, enters the Qin allotment, Chunshou station, sign at wei. Greater Heat — beyond 4°95′16″ of Willow, enters the Zhou allotment, Chunhuo station, sign at wu. End of Heat — beyond 15°56′35″ of Extended Net, enters the Chu allotment, Chunwei station, sign at si. Autumn Equinox — beyond 10°44′5″ of Chariot, enters the Zheng allotment, Shouxing station, sign at chen. Frost Descent — beyond 1°77′77″ of Root, enters the Song allotment, Dahu station, sign at mao. Lesser Snow — beyond 3°97′92″ of Tail, enters the Yan allotment, Ximu station, sign at yin. Winter Solstice — beyond 4°36′66″ of Dipper, enters the Wu-Yue allotment, Xingji station, sign at chou. Greater Cold — beyond 2°91′91″ of Woman, enters the Qi allotment, Xuanxiao station, sign at zi.
107
To find the time of entering the palace.
108
宿
Set each palace-entry lodge degree with fen and miao, subtract that day's before-dawn solar degree, and find where the remainder falls within one degree. Multiply the remainder's fen by the day factor, carry the miao below and multiply through likewise to form the dividend; use that day's solar motion fen as divisor; divide; then seek by emission-and-absorption timing to obtain that day's solar palace-entry time with fen and miao.
109
○ Procedure for Gnomon and Clepsydra, Fourth.
110
Central limit: 182 days, 62 fen, 18 miao.
111
Winter-solstice initial limit, summer-solstice final limit: 62 days, 20 fen.
112
Summer-solstice initial limit, winter-solstice final limit: 120 days, 42 fen.
113
Winter-solstice geocentric gnomon-shadow constant: 1 zhang 2 chi 8 cun 3 fen.
114
Summer-solstice geocentric gnomon-shadow constant: 1 chi 5 cun 6 fen.
115
Circumference factor: 1,428.
116
Inner-outer factor: 10,896.
117
Half factor: 2,615.
118
Day factor, three-fourths: 3,922.5.
119
Day factor, one-fourth: 1,307.5.
120
Dusk-and-dawn fen: 130 fen, 75 miao.
121
Dusk-and-dawn ke: 2 ke, 156 fen, 90 miao.
122
Ke factor: 313 fen, 80 miao.
123
Miao mother: 100.
124
To find the noon mid-accumulation within qi.
125
Set the sought day's greater remainder and half factor, subtract the entered qi's greater and lesser remainders, and obtain that day's noon entry into qi. Add that to the qi mid-accumulation to obtain the day's noon mid-accumulation. Divide the lesser remainder by the day factor to obtain approximate fen.
126
To find noon entry into initial and final limits after the two solstices.
127
Set the noon mid-accumulation and fen; at or below the central limit counts as after winter solstice. If above, subtract the central limit — after summer solstice. Within each solstice period, at or below the initial limit counts as the initial limit. If above, cover and subtract the central limit; the remainder is entry into the final limit.
128
To find the noon gnomon-shadow fixed number.
129
滿滿 滿滿
After winter solstice in the initial limit or after summer solstice in the final limit: multiply the day count by one hundred, include the fen, square the product, and set it aside. Divide by 1,450, add the quotient to 50,380, and combine with half the limit fen; divide the subsidiary by that sum to obtain fen. Ten fen make one cun and ten cun one chi; subtract from the winter-solstice geocentric gnomon-shadow constant to obtain the sought gnomon-shadow fixed number. After summer solstice in the initial limit or after winter solstice in the final limit: multiply the day count by one hundred, include the fen, and square the product for the upper position. Set the entered limit fen below, multiply by 225, reduce by one hundred, and add 198,075 to form the divisor. When before or after summer solstice the value reaches half the limit or above, subtract half the limit and place the result in the upper position. Set half the limit below. In each case multiply the day count by one hundred with the fen included, subtract first, then multiply. Divide by 7,700, add the quotient to the divisor, and divide the upper position to obtain fen; ten fen make one cun and ten cun one chi; add to the summer-solstice geocentric gnomon-shadow constant to obtain the sought gnomon-shadow fixed number.
130
To find the gnomon shadow at each of the four directions.
131
At each place measure the winter and summer solstice gnomon shadows; their difference is that place's solstice gnomon difference. Subtract the geocentric solstice gnomon figures likewise to obtain the geocentric solstice gnomon difference. When the sought day falls after winter solstice in the initial limit or after summer solstice in the final limit: if at or below half the limit, double it; if above half the limit, cover and subtract half the limit and double the remainder, combine with the entered limit days, multiply by three and halve, take days as fen and ten as cun, and subtract from the geocentric solstice gnomon difference to form the divisor. Set the geocentric winter-solstice gnomon-shadow constant, subtract the sought day's geocentric gnomon-shadow fixed number, and multiply the remainder by that year's solstice gnomon difference for the dividend. Divide the dividend by the divisor and subtract the quotient from that place's winter-solstice gnomon figure to obtain that place's gnomon-shadow fixed number for the day. When the sought day falls after summer solstice in the initial limit or after winter solstice in the final limit: if at or below half the limit, double it; if above half the limit, cover and subtract half the limit and double the remainder, combine with the entered limit days, multiply by three and divide by four, take days as fen and ten as cun, and add to the geocentric solstice gnomon difference to form the divisor. Set the sought day's geocentric gnomon-shadow fixed number, subtract the geocentric summer-solstice gnomon-shadow constant, and multiply the remainder by that place's solstice gnomon difference for the dividend. Divide the dividend by the divisor and add the quotient to that place's summer-solstice gnomon figure to obtain that place's gnomon-shadow fixed number for the day.
132
Twenty-four qi ascension–descension and sunrise fen.
133
Ascension–descension rates before and after the two equinoxes.
134
Three days before the vernal equinox the sun enters inside the equator, and three days after the autumnal equinox it emerges outside it — so its ascension and descension diverge from ordinary days; separate rates are therefore assigned for each period.
135
Awakening of Insects, day twelve: ascend 467, 116 — the final rate; use ends here. The decrease-difference likewise ends here. Day thirteen: ascend 441, 6. Day fourteen: ascend 436, 90. Day fifteen: ascend 41.
136
Autumnal Equinox, first day: descend 438. Day one: descend 439. Day two: descend 457. Day three: descend 468. This is the initial rate; use begins here. The increase-difference likewise begins here.
137
To find the daily exit and entry, dawn and dusk, and half-daylight fen.
138
Take the ascension–descension initial rate for each qi, subtract ascension and add descension to that qi's first-day sunrise fen, and obtain the sunrise fen for the day below. Apply the increase-decrease difference and continue adding and subtracting the adjustment difference. Adjust the ascension–descension rate and stepwise accumulate the additions and subtractions to obtain the daily sunrise fen. Cover and subtract the day factor; the remainder is sunset fen. Halve the sunrise and sunset fen together to obtain half-daylight fen. Subtract dusk-and-dawn fen from sunrise fen for dawn fen; add it to sunset fen for dusk fen.
139
To find the double-hours and ke of exit and entry.
140
滿滿
Set the exit-and-entry fen, multiply by six, and divide by the chen divisor for the chen count; divide any remainder by the ke factor for ke, with the unfilled portion as fen; count outward from zi zheng to obtain the result.
141
To find day and night ke.
142
滿
Set sunrise fen, multiply by twelve, and divide by the ke factor for ke, with the unfilled portion as fen — that is night ke. Cover and subtract from one hundred ke; the remainder is day ke.
143
To find the geng and point rates.
144
退 退
Set dawn fen, multiply by four, and step back one place to obtain the geng rate. Multiply the geng rate by two and step back one place to obtain the point rate.
145
To find the double-hour and ke where a geng or point falls.
146
滿 滿滿
Set the geng or point rate, multiply by the sought number of geng or points and again by six, add dusk-and-dawn fen within, and divide by the chen divisor for the chen count. Divide any remainder by the ke factor for ke, with the unfilled portion as fen, and count outward from that chen and ke to obtain the result.
147
To find the clepsydra graduations at each of the four directions.
148
退
At each place run the water clepsydra to fix the winter- or summer-solstice night ke, subtract it from fifty ke, and take the remainder as the solstice-difference ke. Set the sought day's ecliptic distance inside or outside the equator with fen, multiply by the solstice-difference ke and advance one place, divide by 239 for ke, convert any remainder through the ke factor into fen, subtract within and add without fifty ke for night ke, and subtract from one hundred ke for day ke. The day's exit-and-entry chen and ke, together with the geng and point differential rates and related reckonings, are all found by the same procedures.
149
To find ecliptic inner and outer degrees.
150
滿退
Set sunrise fen; if it reaches one-fourth of the day factor or above, remove that portion — the remainder is outer fen. If it falls at one-fourth of the day factor or below, cover and subtract — the remainder is inner fen. Set inner and outer fen, multiply by one thousand, divide by the inner-outer factor for degrees, and convert any remainder into fen — the ecliptic distance inside or outside the equator. Subtract within and add without the quadrant limit to obtain the inner path's distance from the pole.
151
To find the distance-from-center degree and the geng differential degree.
152
退
Set the half factor and subtract dawn fen; multiply the remainder by one hundred and divide by the circumference factor for distance-from-center degrees. Subtract from 183°12′84″, multiply the remainder by four, and step back one place to obtain the differential degree for each geng.
153
To find the culmination stars at dusk, dawn, and the five geng.
154
宿 宿
Set the distance-from-center degree, add that day's noon equatorial solar degree and assign the mansions — the lodge of dusk culmination, which is also the first-geng culmination star. Add the geng differential degree cumulatively, assign the equatorial mansions and cast out full circuits — thus obtain the culmination stars for each successive geng and at dawn.
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