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卷五十八 新五代史考第一

Volume 58 Examination on the New Five Dynasties :

Chapter 58 of 新五代史 · New History of the Five Dynasties
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1
Alas, I find nothing in the rites, music, or literary culture of the Five Dynasties that I would wish to take as a model. Still, later generations who wish to understand that era must not be left without a record. I therefore wrote the "Examination of the Director of Heaven and the Director of Regions." ○ Part One: Examination of the Director of Heaven
2
使
The Director of Heaven was charged with observing the sun, moon, stars, and constellations. One circuit of heaven marks a year, divided into four seasons, twenty-four qi, seventy-two hou, and measured by the ten-day week and twelve double-hours—this is what the calendar records. Careful observation of their variations yields material for divination. Divination reads extraordinary signs to test good and ill fortune, discern Heaven's will, and guide human affairs; its methods were entrusted to the appropriate offices. The calendar rests on fixed numerical cycles to project cold and heat, anticipate the heavenly pattern, and regulate human affairs; its methods commanded universal trust. Astronomical techniques may be applied as needed, yet calendrical rules must not deviate even for one day. A deviation no wider than a hair's breadth can throw Heaven and humanity out of order and upset the timing of every affair of state—which is why rulers treated it with such gravity. Still, from Yao's appointment of Xi and He in the Documents, the cardinal stars and intercalary remainders preserve at least the broad outline of the original method. Yet across the thousand-odd years of the Three Dynasties, the transmitted records fell into neglect, and the Six Classics say nothing on the subject. Nor did Confucius and his disciples ever address it. In later times the subject passed entirely into the hands of the yin-yang specialists: the office remained weighty, but the learning had become a minor craft. The boundary between Heaven and humanity is immeasurably remote and subtle, yet technicians of a single craft would lay out counting-rods and accumulated fractions, reaching back tens of millions of years until they fixed a jiazi year in which new moon, dawn, midnight, and winter solstice aligned, with sun, moon, and the five planets all gathered at zi—the "supreme origin" taken as the calendar's starting point. Only from the Han onward did this doctrine appear in full; its origins extend no further back than this. Can this really have been the method of Yao, Shun, and the Three Dynasties? None of it can be verified by evidence. Yet from that time on, though calendrical schools differed from one generation to the next, none ever departed from this foundation.
3
調 調
At the outset of the Five Dynasties period, the court continued Tang practice and adopted the Chongxuan Calendar. Under Jin Emperor Gaozu, Director of Heaven Ma Chongji devised a new calendar that abandoned retrojection to the ancient supreme origin of jiazi, winter solstice, and the seven luminaries in conjunction, and instead took yiwei, the fourteenth year of Tang's Tianbao era, as the supreme origin, with Rain Water in the first month as the year's qi-head. Earlier, during Tang's Jianzhong era, the technician Cao Shibian had first broken with ancient practice, taking the fifth year of Xianqing as the supreme origin and Rain Water as the year's beginning—the calendar known as the Futian Calendar. The world called it the "minor calendar," and it circulated only among commoners. Chongji adopted it as the official standard, and the court promulgated it under the title Tiaoyuan Calendar. After only five years it had drifted out of alignment and was abandoned, and the Chongxuan Calendar was restored. During Later Zhou's Guangshun era, National University academician Wang Chune privately composed the Mingxuan Calendar at home. Commoners also used the Wanfen Calendar; Shu had the Yongchang and Zhengxiang calendars; Southern Tang had the Qizheng Calendar. For the Five Dynasties period, the calendrical traditions that can be documented end here. The Tiaoyuan method was already unorthodox; the Mingxuan never left Wang's household; the Wanfen never left the folk sphere—none of their methods merit recording. The Yongchang, Zhengxiang, and Qizheng calendars were each confined to its own state; all are now lost and no longer extant.
4
殿
When Emperor Shizong came to the throne, he campaigned abroad against rebel regimes while reforming laws and institutions at home. Hanlin academician Wang Pu, who was expert in calendrical reckoning, received an imperial order to draft a new calendar. After more than a year, Pu submitted a memorial that read:
5
◎ Your servant has heard that what the sage establishes rests on understanding the transformations of Heaven and humanity. The movements of human affairs can be grasped through language; but the movements of the Heavenly Way must be grasped through numbers. It is through number that the sage observes the Heavenly Way. Years, months, days, and hours take their form thereby; yin and yang, cold and heat, are regulated thereby; and the governance of the four quarters proceeds thereby. Whoever governs a state, in inaugurating the year and establishing the cosmic pole, must embody its origin; in promulgating policy and assessing achievement, must follow the year's cycle; in performing rites and music, must align the new moon; farmers and artisans alike must follow its seasons; punishments and punitive campaigns must follow its qi; every affair of state must follow its sun and moon. Therefore when the sage receives the Mandate, he must set the calendar in order. Thus the five chronologies hold their fixed measures, the various portents their fixed responses, and the correct calendar is promulgated throughout the realm.
6
From the end of Tang through successive dynasties, the calendar fell into chaos and Heaven's order was lost; for nearly a century the heavenly reckoning lay in ruins. Your Majesty has followed the ancient Way, stood in reverent awe of Heaven, consulted his officials, and revived fallen institutions. Though your servant lacks ability, how could I dare refuse the imperial command? I have embraced the myriad phenomena as method, aligned the seven regulators to establish the origin, measured the gnomon and clepsydra to observe the qi, examined lunar elongation to fix the new moon, clarified the nine paths to track the moon, calibrated planetary motion to project the stars, investigated the obliquity of the ecliptic, distinguished the rising and falling of celestial disposition, and rendered eclipses precise.
7
退
The Way established for Heaven is yin and yang. Yin and yang each have their numbers; combined, they produce transformation and completion. The yang tally is thirty-six; the yin tally, twenty-four. Odd and even are paired by command: two yang and three yin alike yield seventy-two. When they match, the numbers of yin and yang unite. Seventy-two is the number of transformation and completion. Transformation and completion constitute the numbers of the Five Phases. Multiply by five to obtain the period number. What exceeds is called qi surplus; what falls short is called new-moon deficit. In responding to change and apportioning use, nothing lies beyond its reach. Therefore seventy-two serves as the canonical method. The canonical method is that in constant use. One hundred is the node of numbers; advancing and retreating with the method without losing position—hence the universal method. Advancing the canonical by the universal method yields 7,200—the comprehensive method. From the origin through the canonical, this method is applied first—it governs all methods of the comprehensive calendar. Advancing the comprehensive by the universal method yields 720,000. Beneath qi and new moon, when collected fractions are fully exhausted, this is the complete rate. Advancing the complete rate by the universal method yields 72 million—the great rate, from which the origin and era are born. The origin is when year, month, day, and hour are all jiazi; sun, moon, and the five planets all gather at zi; standing at the mean of expansion and contraction, precedence and lag—what is called the seven regulators in alignment.
8
使
In antiquity the gnomon was erected at Yangcheng because it lay near the Luo. Still dissatisfied with its centrality, they placed it on the Luo's eastern margin. In Kaiyuan 12, envoys were dispatched empire-wide to observe shadows, from Linyi in the south to Hengye in the north; at the center they found the Yuetai at Junyi, on the north-south meridian at the earth's midpoint. When Great Zhou established its state, it fixed the capital at Bian. The gnomon was erected and clepsydra arrows set; the Yuetai sundial and water-clock were measured to establish the central reckoning. When sundial and water-clock are correct, the sun's position and the qi's response can be determined.
9
Both sun and moon exhibit expansion and contraction. When the sun expands and the moon contracts, the median lags and the new moon follows. When the moon expands and the sun contracts, the median comes early and the new moon precedes. From antiquity, methods for lunar elongation relied on uniform-motion numbers; though entering the calendar already had prior sequences, the gradations of increase and decrease were inconsistent. The old Huangji method was circuitous and impractical. Later calendars were crude and prone to error. Now lunar elongation is calibrated against the calendar, and solar motion receives additions and subtractions at the point of application. What is obtained is the day fixed by entering departure. A single day is divided into nine limits. Each limit has its increase and decrease; the gradations follow a coherent order. The method for lunar elongation may truly be called precise.
10
宿 宿宿 宿宿 宿 使
The celestial equator is Heaven's girding belt. Circular and level in form, it records the constant lodge degrees. The ecliptic is the sun's track. Half lies within the equator, half outside, twenty-four degrees from the pole. When near the equator, its course is oblique; when far from the equator, its course is straight. When oblique, the sun's daily motion should be slow; when straight, the sun's daily motion should be fast. Accordingly, degrees are added before and after the equinoxes and subtracted before and after the solstices. The nine paths are the moon's orbit. Half lies within the ecliptic, half outside, six degrees farther from the pole. Emerging from the ecliptic is called the primary crossing; entering the ecliptic is called the median crossing. If the primary crossing falls at the autumn-equinox lodge and the median at the spring-equinox lodge, the orbit is more oblique than the ecliptic. If the primary crossing falls at the spring-equinox lodge and the median at the autumn-equinox lodge, the orbit is conversely straighter than the ecliptic. If both crossings fall at the solstice lodges, the orbit is moderately oblique. By calibrating distance from the solstices and equinoxes to test obliquity and rectitude, one obtains the numbers for addition and subtraction. Although the nine paths were discussed from antiquity, the tradition knew them only in outline—texts handed down by rote, without computational use. The ecliptic's full circuit is now divided into eight nodes; each node is divided into nine paths; yielding seventy-two paths in all, so that sun and moon conceal nothing of their oblique and straight courses. The method of the nine paths may truly be called clear.
11
便 退
A planet moves swiftly near the sun and slowly when far from it. At greatest distance from the sun its momentum is spent and it stations. Ancient calendars divided segments inaccurately, with no standard for rise and fall; one day its motion-fraction is still large, the next day it stations; from station it retreats using only uniform motion, still taking segment motion-degrees as the calendar entry number; none of this accords with fundamental principle, and contradiction follows. Daily motion-fractions are now accumulated in sequence to form variable segments. Then from swift it gradually slows until momentum is spent and it stations. From station it proceeds again, accumulating minutely before becoming great. Separate variable segments and variable calendars project the variable differences so that segment differences align in meeting. Planetary slow and swift motion can thereby be known.
12
Tradition held that within fifteen degrees of nodal departure, sun and moon would eclipse. They did not grasp that mutual masking of sun and moon and casting of the dark void follow different principles. By comparing sun and moon diameters, calibrating nodal distance, ecliptic obliquity, celestial disposition, and overhead versus side-view fractions, eclipse magnitude is obtained in reality.
13
Your servant finds no earlier text on the head and tail of the eclipse spirit. Recently, minor techniques of the Director of Heaven and diviners, unable to grasp the whole, devised a method of equal connection. Adopted provisionally for convenience, it gave crossing a retrograde number. Later students, ignorant of the details, said the calendar had nine luminaries as the regular annotating form. All of these are now cut away. Respectfully, "Pacing the Sun," "Pacing the Moon," "Jupiter," and "Pacing the Collector" form four chapters, combined into one fascicle of the 《Calendar Classic》, eleven fascicles of 《Calendar》, three of 《Draft》, and one fascicle of the 《Detailed Motion of the Seven Regulators》 for Xiande 3, as the 《Qintian Calendar》.
14
Of old, Emperor Yao reverently conformed to august Heaven. Your Majesty examines the calendar and the images of sun, moon, stars, and constellations—the Way of Yao and Tang. The Heavenly Way is profound and remote—beyond your humble servant's full knowledge. Emperor Shizong commended it. He ordered the Director of Heaven to adopt it, beginning from new moon and dawn of the first month of the following year. The 《Xiande Qintian Calendar》
15
Projecting the era from supreme origin jiazi to the present Xiande 3 bingchen: accumulated 72,698,452 counts beyond. 《Qintian》 comprehensive method: 7,200. 《Qintian》 canonical method: 72.
16
《Qintian》 universal method: 100. 《Qintian》 method for pacing the sun's motion, year rate: 2,629,760, 40. Track rate: 2,629,844, 80.
17
New-moon rate: 212,620, 28. Year tally: 365, 1,760, 40. Track tally: 365, 1,844, 80. Year median: 182, 4,480, 20.
18
Track median: 182, 4,522, 40. New-moon tally: 29, 3,820, 28. Qi tally: 15, 1,573, 35. Image tally: 7, 2,755, 7.
19
Cycle era: 60. Year difference: 84, 40.
20
宿
Double-hour rule: 600; eight quarters and twenty-four minutes. ◎ Red Path lodge sequence
21
宿
Dipper: 26 degrees. Ox: 8 degrees. Girl: 12 degrees. Void: 10 and a fraction degrees. Rooftop: 17 degrees. Room: 16 degrees. Wall: 9 degrees. The seven northern lodges: 98 and a fraction degrees.
22
西宿
Striding: 16 degrees. Bond: 12 degrees. Stomach: 14 degrees. Mao: 11 degrees. Net: 17 degrees. Turtle Beak: 1 degree. Shen: 10 degrees. The seven western lodges: 81 degrees.
23
宿
Well: 33 degrees. Ghost: 3 degrees. Willow: 15 degrees. Star: 7 degrees. Extended Net: 18 degrees. Wings: 18 degrees. Chariot Shaft: 17 degrees. The seven southern lodges: 111 degrees.
24
宿
Horn: 12 degrees. Gullet: 9 degrees. Base: 15 degrees. Room: 5 degrees. Heart: 5 degrees. Tail: 18 degrees. Winnowing Basket: 11 degrees. The seven eastern lodges: 75 degrees. ◎ Median nodes
25
Set the year rate and multiply by accumulated years from the projecting era's supreme origin to the year sought to obtain qi accumulation. Divide by the comprehensive method to obtain days. Remove full cycle eras; count from jiazi beyond the calculation—the day, double-hour, and fractional parts of the heavenly median qi. Add cumulatively by the qi tally; seconds filling the universal method follow into minutes, minutes filling the comprehensive method into days, days filling the cycle era are removed—each yields the next qi's day, double-hour, and fractional parts.
26
New moon, first quarter, full moon
27
Set the qi accumulation and remove by the new-moon rate; the remainder is intercalary surplus. Subtract it from qi accumulation to obtain new-moon accumulation. Divide by the comprehensive method to obtain days. Remove full cycle eras; count from jiazi beyond the calculation—the day, double-hour, and fractional parts of the heavenly normal new moon. Add cumulatively by the image tally to obtain each quarter, full moon, and successive new moon.
28
Sun's motion entering the calendar
29
滿
Set the year rate, subtract intercalary surplus, and divide by the comprehensive method to obtain days. Below the year median counts as expansion; above it, subtract the year median for contraction—the entry for the heavenly normal new moon's added time. Add cumulatively by the image tally; when full remove from the year; expansion and contraction alternate in naming—the four images' entry.
30
Sun's motion in lunar elongation
31
Set added-time entry calendar fractional parts; multiply by that day's increase-decrease rate; divide by the comprehensive method; adjust that day's elongation number for the sun's fixed elongation number. ◎ Red Path solar degrees
32
宿 宿 宿
Set qi accumulation; remove by track rate; divide remainder by comprehensive method for degrees; count from Void 8 beyond the Red Path calculation—the sun's Red Path lodge degree and fractional parts at heavenly median qi's added time. Add the year median and name in sequence—the summer solstice lodge. ◎ Yellow Path lodge sequence
33
宿 宿 宿 宿宿
Set the Red Path lodge degrees of solar motion at the two solstices. Every five degrees before and after as a limit; initial rate eight, each limit decreasing by one through nine limits, final rate zero; then one degree and a slight surplus, limit rate zero. Its half corresponds to the lodges of the four establishments. Thereafter five degrees as a limit; initial rate zero, each limit increasing by one through nine limits, final rate eight—the equinox lodges. From equinox to solstice, the same applies. Each multiplies limit rate by limit degrees entered for fractional parts. Divide by the canonical method to obtain degrees. Nine limits before and after solstices subtract from, and nine limits before and after equinoxes add to, Red Path lodges for Yellow Path lodges and fractional parts. From fractional parts derive slight, great, and half numbers.
34
Yellow Path solar degrees
35
宿 宿 宿
Set Red Path lodge degree of solar motion at heavenly median qi's added time. Each is multiplied by the limit rate entered, all extended through the comprehensive method; the limit rate entered multiplies its fractional parts and follows along. Divide by the canonical method for fractional parts; when full of comprehensive method, for degrees. Subtract from the Red Path position—the Yellow Path lodge degree and fractional parts at heavenly median qi's added time. Add year median; name by Yellow Path lodge sequence—solar degree and fractional parts at summer solstice added time.
36
Noon solar motion
37
滿 宿
Set solstice fractional parts; subtract half the method for after-noon fractional parts; if insufficient, reverse subtract for before-noon fractional parts. Multiply first day's motion fractional parts; divide by canonical method; before noon add, after noon subtract from added-time Yellow Path degrees—for noon solar degrees. Add each next day's motion fractional parts; when full of comprehensive method follow into degrees. Name by lodge sequence—the next day's noon solar motion.
38
Noon solar motion entering the calendar
39
便 滿
Set heavenly median qi before-noon fractional parts as noon entry expansion calendar day fractional parts. If after noon, subtract after-noon fractional parts from year median for noon entry contraction calendar day fractional parts. Add one day cumulatively; when full of year median remove; expansion and contraction alternate—for each day's noon calendar entry.
40
Yuetai median gnomon shadow
41
Set noon entry calendar fractional parts; multiply by that day's increase-decrease rate; as comprehensive method to one for fractional parts; ten fractional parts make one inch. Increase or decrease the lower median gnomon number for the fixed number. ◎ Dawn and dusk fractional parts
42
Set entry calendar fractional parts; multiply by increase-decrease rate; as comprehensive method to one; adjust lower dawn fractional parts for dawn fixed fractional parts. Decrease to add and increase to subtract lower dusk fractional parts for dusk fixed fractional parts. ◎ Day entry and exit double-hours and quarters
43
滿
Set dawn and dusk fractional parts; add 180 to dawn and subtract from dusk for day entry-exit fractional parts. Each divide by double-hour rule for double-hour numbers; remainder filling canonical method for quarters; count double-hours from zi beyond calculation—day entry-exit double-hours and quarters. ◎ Day and night quarters
44
滿
Set day-entry fractional parts; subtract day-exit for day fractional parts. Subtract from comprehensive method for night fractional parts. Each fills canonical method for day and night quarters. ◎ Five night double-hours and quarters
45
滿滿
Set dusk fractional parts; divide by double-hour rule for double-hour numbers; divide by canonical method for quarter numbers. Count from zi beyond calculation—the first night double-hours and quarters. Double dawn fractional parts; divide by five for watch-use fractional parts. Again divide by five for tally-use fractional parts. Add cumulatively to first night; when full of double-hour rule for hours, full of canonical method for quarters—five nights' double-hours and quarters.
46
Median stars at dusk and dawn
47
Set dusk fractional parts; subtract half comprehensive method; multiply by track rate; divide by comprehensive method for distance-from-median fractional parts. When full of comprehensive method, for degrees. Add to noon solar motion for dusk median star; subtract for dawn median star. ◎ Red Path inner and outer numbers
48
Set entry calendar fractional parts; multiply by increase-decrease rate; as comprehensive method to one; adjust lower inner-outer numbers; if insufficient to decrease, reverse the decrease; inner and outer alternate in naming—for sought Red Path inner-outer fixed number. ◎ Nine domains' distance-from-track numbers
49
Set li distance north and south from Yuetai; extend through by 360 for paces. Divide by 1,756; north add, south subtract 2,513 for girdle-median number; with Red Path inner-outer fixed number, inner subtract outer add—for nine domains' distance-from-track number.
50
Nine domains' median gnomon
51
Set distance-from-track number; multiply by 25; divide by 137 for heaven-use fractional parts. Set it; multiply by 22; divide by six; subtract 4,000 for gnomon method. Self-multiply heaven-use fractional parts; as gnomon method to one for earth-use fractional parts. Follow together for gnomon fractional parts; ten parts make one inch—that place's median gnomon.
52
Nine domains' clepsydra gradations
53
Extend comprehensive method through track median and halve; self-multiply; as that place's girdle-median number to one; multiply by 263; divide by canonical method for clepsydra method. Extend track median above; set Red Path inner-outer below; subtract below from above; multiply remainder; when full of clepsydra method, for clepsydra fractional parts. Within Red Path subtract, outside add 1,620 for that place's dawn fractional parts. Subtract from comprehensive method for dusk fractional parts. Set dawn and dusk fractional parts; each enter by Yuetai technique—for that place's day entry-exit, five nights, and dusk-dawn median stars.
54
《Qintian》 method for pacing lunar departure, departure rate: 198,393, 9. Crossing rate: 195,927, 97, 56. Departure tally: 27, 3,993, 9.
55
Crossing tally: 27, 1,527, 97, 56. Full-moon tally: 14, 5,510, 14. Crossing median: 13, 4,363, 98, 78. Departure new moon: 1, 7,027, 19.
56
Crossing new moon: 2, 2,292, 30, 44. Median standard: 1,736. Median limit: 4,780. Level departure: 963.
57
Procedure interval: 800. ◎ Lunar departure: entering the calendar
58
滿
Set new-moon accumulation, remove the departure rate, and take days as the remainder over the comprehensive method—the calendar entry at added time for the heavenly normal new moon. Add the image tally cumulatively, removing full departure tallies, to obtain calendar entries for quarters, full moons, and successive new moons. ◎ Lunar departure: elongation correction
59
Set calendar-entry fractional parts; apply the sun's fixed elongation number—subtract for waning elongation, add for waxing—and divide by the procedure interval to obtain the limit number. Multiply the remainder by the limit's increase-decrease rate, divide by the procedure interval, and adjust the limit elongation to obtain the fixed number. ◎ Fixing the days of new moon, quarters, and full moon
60
退
For each phase, apply the fixed solar and lunar elongation numbers—subtract for waning, add for waxing—to the constant fractional parts to obtain the fixed day. If the sun has already set at the computed time of the fixed new moon, advance the date by one day; unless an eclipse is visible at its beginning—in which case do not advance. For a quarter or full moon whose added time falls before sunrise, retreat one day; the same applies if an eclipse is visible at its beginning even when the sun has already risen. When the year's first day bears a crossing, fix the intercalation by the waxing-and-waning rule. If the fixed new moon and the next new moon share the same celestial stem, the month is long; if they differ, it is short; A month without a median qi is intercalary.
61
Solar longitude at added time for new and full moon
62
宿
Set the sun's calendar entry and adjust it with the fixed solar and lunar elongation numbers—subtract for waning, add for waxing—to obtain the calendar entry at fixed-new-moon added time. Multiply calendar fractional parts by that day's increase-decrease rate, divide by the comprehensive method, and adjust the lower expansion-contraction figure to obtain the fixed number. Set the fixed-new-moon calendar fractional parts, reduce by the universal method, and add for expansion or subtract for contraction according to the fixed number. Count lodge positions from the winter and summer solstice starting points to obtain the result sought.
63
Lunar departure: entering the crossing
64
滿
Set new-moon accumulation, remove the crossing rate, and take days as the remainder over the comprehensive method—the general crossing day for the heavenly normal new moon. Add the full-moon tally cumulatively, removing full crossing tallies, to find entries for the full moon and successive new moons. Apply the sun's fixed elongation number—subtract for waning, add for waxing—to obtain the constant crossing day. Set the lunar fixed elongation number, multiply by the canonical method, divide by level departure, and subtract or add to the constant fractional parts to obtain the fixed crossing day.
65
Ecliptic longitude at rectified crossing
66
宿 宿
Extend fixed crossing days through the comprehensive method, multiply by 254, and divide by 19. Divide again by the comprehensive method to obtain crossing-entry degrees. Subtract from the new-moon added-time solar longitude to obtain the moon's ecliptic lodge position at rectified crossing before new moon. ◎ Lodge sequence of the nine paths
67
宿 宿 宿 宿 宿 宿 宿 宿宿 宿宿 宿
Lunar departure crosses the ecliptic by six degrees. The variation follows the eight nodal points, with differing obliquity and alignment. Hence the moon's motion comprises nine paths. Each of the eight ecliptic nodal points has nine limits. From rectified crossing, the lodge of the first limit after each node marks the moon's first path in that node. The lodge where the second limit begins marks the second path, and that starting limit becomes the first limit after rectified crossing. The initial rate is eight, decreasing by one per limit through nine limits, with a final rate of zero. Nine more limits follow, rising from zero to eight and approaching the lodge of half crossing. Another nine limits then descend from eight to zero in the same manner. Nine limits rise again from zero to eight until the path rejoins the ecliptic—the median crossing. The segment from median to rectified crossing follows the same pattern. Set the limit degrees entered and multiply by the limit rate to obtain the general difference. For the nine limits before and after rectified and median crossing, multiply by the solstice limit count. For the nine limits before and after half crossing, multiply by the equinox limit count; divide each by the canonical method to obtain the ecliptic difference. After the winter-solstice lodge, subtract for nine limits around rectified crossing and add for nine limits around median crossing. After the summer-solstice lodge, add for nine limits around rectified crossing and subtract for nine limits around median crossing. In general, after rectified crossing the moon lies outside the ecliptic; after median crossing it lies within. For nine limits around half crossing: after the spring-equinox lodge, exiting the ecliptic, and after the autumn-equinox lodge, entering within—all add the difference; After the spring-equinox lodge, entering within, and after the autumn-equinox lodge, exiting without—all subtract the difference. Reduce the general difference by one quarter and subtract the ecliptic difference to obtain the equatorial difference. For nine limits around rectified and median crossing, always add the difference. For nine limits around half crossing, always subtract the difference. Apply the two ecliptic and equatorial differences to the ecliptic to obtain the nine-path lodge sequence; Express the fractional parts as slight, great, and half. Eight nodal points times nine paths yield seventy-two paths completing the cycle.
68
Lunar position on the nine paths at rectified crossing
69
宿 宿
Set the moon's ecliptic lodge position at rectified crossing; Multiply by the entered limit rate and its fractional parts, reduce by the canonical method, to obtain the general difference. Derive the ecliptic and equatorial differences and apply them to obtain the moon's nine-path lodge position at rectified crossing. ◎ New-moon lunar position on the nine paths
70
宿宿宿
Set the moon's nine-path position at rectified crossing, add crossing-entry degrees, and count through the nine-path sequence for the lunar nine-path position at new-moon added time. ◎ Full-moon lunar position on the nine paths
71
宿
Set the solar separation at new- and full-moon added time, add track median, to obtain the added-time image accumulation. Add this to the new-moon nine-path lunar position and count through that path's lodge sequence to obtain the result. Project backward from full moon to new moon by the same method. ◎ Lunar departure: noon calendar entry
72
Set lunar calendar entries for new and full moon, add half the comprehensive method and subtract fixed fractional parts, then adjust with fixed solar and lunar elongation—subtract for waning, add for waxing—to obtain the result. ◎ Dawn and dusk lunar positions
73
滿
Set that day's dawn and dusk fractional parts and subtract the fixed parts to obtain the before fraction; if insufficient, reverse the subtraction to obtain the after fraction. Multiply by that day's departure procedure, divide by the comprehensive method, and convert fractions filling the canonical method into degrees for dawn and dusk offsets. add for before and subtract for after from the added-time lunar position to obtain dawn and dusk lunar positions.
74
Image accumulation at dawn and dusk
75
Set the added-time image accumulation, apply the prior image's before-after degrees (subtract before, add after), then the latter image's degrees (add before, subtract after), to obtain the result. ◎ Daily dawn and dusk lunar positions
76
宿
Accumulate departure degrees from the following image and subtract from the dawn-dusk image accumulation for addition; if insufficient, reverse the subtraction for subtraction. Divide by the days to the following image and apply to adjust each day's departure degrees to obtain fixed degrees. Add dawn and dusk lunar positions cumulatively and count through the nine-path lodge sequence to obtain the result.
77
Lunar latitude relative to the ecliptic
78
滿
Set the fixed crossing day. Below the crossing median, the moon travels the yang path; above it, subtract to obtain the yin path—extend both through the canonical method. subtract from 980, multiply the remainder, and divide by 556 for fractional parts; and convert to degrees when the canonical method is filled. on the yang path, outside the ecliptic; on the yin path, inside the ecliptic—the lunar latitude sought.
79
Solar and lunar eclipse limits
80
Set the fixed day on the yin or yang crossing path. Below half the crossing median counts as after crossing; above, subtract from the crossing median for before crossing—extend both through the comprehensive method as distance-from-crossing parts. At new moon, if distance-from-crossing parts are 4,219 or less on the yang path or 10,383 or less on the yin path, a solar eclipse is possible. At full moon, if distance-from-crossing parts are 6,995 or less on either path, a lunar eclipse is possible.
81
Fixed fractional parts for eclipse maximum time
82
Set the fixed fractional parts for new moon. If above half the comprehensive method, subtract half the comprehensive method; if below, subtract from half the comprehensive method to obtain distance-from-noon parts. Multiply by eleven and divide by the canonical method. If below half the comprehensive method, subtract it; if above, add to the new-moon fixed parts—to obtain fixed fractional parts for solar-eclipse added time. When the value lies above [half comprehensive], add the new-moon fixed fraction to obtain the fixed fraction for the hour of greatest solar eclipse. For full moon, subtract the day's morning fraction from 1,620, multiply the remainder by 245, and divide by 313; subtract that from 245, then add or subtract the remainder to the full-moon fixed fraction to obtain the fixed fraction for the hour of greatest lunar eclipse.
83
Constant standard for solar eclipses
84
Place the median standard; multiply it by the day's equatorial inner-or-outer index, divide by 2,513, and obtain the ecliptic ingress–egress eclipse correction. multiply by (half daytime fraction minus distance-from-noon fraction), then divide by half the daytime fraction; subtract from the median standard when inside the equator, add when outside—this yields the solar eclipse constant standard.
85
Fixed standard for solar eclipses
86
Set solar motion's circuit entry, convert by the canonical method; if below 3,287, subtract from 3,287—this is post-solstitial; if above, subtract 3,287—this is pre-equinoxial. If above 6,574, subtract from 9,861—this is post-equinoxial; if above, subtract 9,861—this is pre-solstitial. Divide each by three; subtract for solstitial intervals, add 2,772 for equinoctial intervals—this is the ecliptic obliquity eclipse correction. Multiply by distance-from-noon, divide by half daytime, add to the constant standard to obtain the fixed standard.
87
Magnitude of solar eclipse
88
Add the fixed standard to the median limit to obtain the yin-path fixed standard; subtract the median limit to obtain the yang-path fixed limit. If subtraction is impossible, subtract in reverse—this is the beyond-limit fraction. For yin-path distance-from-crossing: when fixed standard exceeds and fixed limit is not exceeded, a yin-path eclipse applies; set the fixed limit and subtract distance-from-crossing to obtain distance-from-eclipse. Below the fixed standard, though nominally yin-path, treat as yang-path eclipse; add the yang-path fixed limit to obtain distance-from-eclipse. If a beyond-limit fraction exists, subtract it to obtain distance-from-eclipse. If subtraction fails, no eclipse occurs. For yang-path distance-from-crossing below the fixed limit, the eclipse enters the fixed limit; subtract it from the yang-path fixed limit to obtain distance-from-eclipse. Set each distance-from-eclipse fraction and divide by 478 to obtain the solar eclipse major fraction; the remainder is the minor fraction. Express the major fraction in tenths; express the minor fraction in halves and strong/weak gradations.
89
Magnitude of lunar eclipse
90
Inspect distance-from-crossing: at or below the median standard, the eclipse is total; above that, subtract from the eclipse limit to obtain distance-from-eclipse. Set the value and divide by 526 for the lunar eclipse major fraction; the remainder is the minor fraction. Express the major fraction in tenths; express the minor fraction in halves and strong/weak gradations.
91
General-use fraction for solar eclipse timing
92
Set distance-from-eclipse; if 1,912 or greater, subtract from 4,780; multiply the remainder by itself and divide by 63,272; subtract the result from 647 to obtain the general-use fraction. If 956 or less, subtract from 1,912, multiply the remainder by the universal method, and divide by 735; subtract from 517 to obtain the general-use fraction. If 956 or greater, square distance-from-eclipse and divide by 2,362; subtract from 387 to obtain the general-use fraction.
93
General-use fraction for lunar eclipse timing
94
Set distance-from-eclipse; if 2,140 or greater, subtract from 5,260; multiply the remainder by itself and divide by 69,169; subtract from 711 to obtain the general-use fraction. If 1,052 or greater, subtract from 2,140; divide the remainder by 7; subtract from 567 to obtain the general-use fraction. If 1,052 or less, subtract distance-from-eclipse; multiply the remainder by itself and divide by 2,654; subtract from 417 to obtain the general-use fraction.
95
Fixed fractions for the added times of eclipse first contact and last contact
96
Set each general-use fraction, multiply by mean departure, divide by the day's departure interval to obtain the fixed-use fraction. Subtract it from the syzygy fixed fraction to obtain first contact. Add it to obtain last contact. Apply the added-time constant fraction by the greatest-eclipse procedure to obtain fixed times for first and last contact. Set the first-contact, greatest, and last-contact fixed fractions; divide each by the double-hour divisor to obtain the double-hour; divide the remainder by the canonical method for quarters—the double-hours and quarters of first contact, maximum, and last contact.
97
Direction of eclipse onset
98
西
Solar eclipses first contact in the west; lunar eclipses first contact in the east. For small magnitude, when the Moon is on the yang path, solar eclipses skew south and lunar eclipses north; on the yin path, solar eclipses skew north and lunar south—these are the standard constants. From after Lichun to before Lixia, large eclipses bias solar south and lunar north; from after Liqiu to before Lidong, large eclipses bias solar north and lunar south—this follows ecliptic obliquity. Yang path before the node and yin path after it, large eclipses bias solar south and lunar north; yang path after the node and yin path before it, large eclipses bias solar north and lunar south—this follows lunar-path obliquity. Ecliptic deviation from the standard constants is smaller; lunar-path deviation from the ecliptic is a further quarter—all reckoned from local noon. For morning or afternoon, one rule skews south and one north; combine eclipse magnitude with seasonal phase to fix the azimuths of first contact, maximum, and last contact—each desired result then follows.
99
Fraction for eclipses at sunrise or sunset
100
If the day's sunrise/sunset fraction falls between the first-contact and last-contact fixed fractions, the eclipse occurs at rising or setting. If greatest eclipse precedes sunrise/sunset, subtract the exit-and-entry fraction from the last-contact fixed fraction for the horizon correction. If greatest eclipse follows sunrise/sunset, subtract the exit-and-entry fraction from the first-contact fixed fraction for the horizon correction. Set each horizon correction, multiply by distance-from-eclipse, divide by fixed-use fraction, then divide by 478 for solar or 526 for lunar eclipses to obtain the horizon eclipse major fraction; the remainder is the minor fraction.
101
Night watches and clepsydra tallies of the eclipse
102
Set the first-contact, greatest, and last-contact fixed fractions. When below the morning fraction, add the evening fraction; if above the evening fraction, subtract it; divide each by the watch divisor to obtain the watch count. Divide the remainder by the tally divisor to obtain the clepsydra tally count.
103
《Qintian》 procedure for the five planets ◎ Jupiter circuit rate: 2,871,976, 6. Variation rate: 242,215; remainder 66.
104
Calendar rate: 2,629,761; remainder 78. Circuit tally: 398 days, 6,376 parts, remainder 6. Circuit median: 182, 4,480, 89. Variable segment, variable days, variable degrees, variable calendar
105
Morning appearance: 17 days, 3 parts (37)〉 2 [parts] (24)〉
106
Swift direct motion: 91 days, 16 parts (63)〉 11 [parts] (13)〉
107
Direct slow motion: 25, 2. 9 1 (29)〉 Station before retrograde: 26. (32)〉
108
退
Retrograde slow motion: 14, 1. (12)〉 zero (blank entry) (28)〉
109
退
Retrograde fast motion: 27, 4. (38)〉 1 (37)〉
110
退
Retrograde fast motion: 27, 4. (38)〉 1 (37)〉
111
退
Retrograde slow motion: 14, 1. (12)〉 zero (blank entry) (28)〉 Station after retrograde: 26. (32)〉
112
Direct slow motion: 25, 2. 9 1 (29)〉
113
Direct fast motion: 91, 16. (63)〉 11 (13)〉
114
Evening disappearance: 17, 3. (37)〉 2 (24)〉 ◎ Mars orbital cycle rate: 5,615,422; remainder 11. Mutation rate: 2,985,661; remainder 71.
115
Calendar rate: 2,629,760; remainder zero. Circuit tally: 779; 6,622; remainder 11. Mid-cycle: 182; 4,480; remainder zero. Mutation segment | mutation days | mutation degrees | mutation calendar.
116
Morning appearance: 73, 53. (68)〉 50 (58)〉 Direct fast motion: 73, 51. 1 48 3
117
Second direct-fast phase: 71, 46. (69)〉 44 (17)〉
118
Second direct-slow phase: 71, 45. (33)〉 42 (58)〉 Direct slow motion: 62, 19. (29)〉 18 (20)〉 Station before retrograde: 8. (69)〉
119
退 退 退
Retrograde slow motion: 11. (58)〉 zero (blank entry) (44)〉 Retrograde fast motion: 21, 7. (46)〉 2 (40)〉 Retrograde, swift: 21 days, 7 degrees (46)〉 2 (40)〉
120
退
Retrograde, slow: 11 days, 1 degree (58)〉 (44)〉 Latter station: 8 days (69)〉 Prograde, slow: 62 days, 19 degrees (29)〉 18 (20)〉
121
Secondary slow: 71 days, 45 degrees (33)〉 42 (58)〉
122
Secondary swift: 71 days, 46 degrees (69)〉 44 (17)〉 Prograde, swift: 73 days, 51 degrees fraction 1 48 fraction 3
123
Evening hiding: 73 days, 53 degrees (68)〉 50 (58)〉 ◎ Saturn cycle rate: 2,722,176; remainder 90. Variation rate: 92,416; remainder 50.
124
Calendar rate: 2,629,759; remainder 80. Sidereal period: 378 days; remainder 576; fraction 90. Mid-cycle: 182 days; remainder 4,479; fraction 90. Segment | Days | Degrees | Calendar
125
Morning appearance: 19 days, 2 degrees fraction 7 1 (14)〉 Prograde, swift: 65 days, 6 degrees (38)〉 3 (51)〉 Prograde, slow: 19 days; degrees — (63)〉 (35)〉
126
退 退 退
Prior station: 37 days fraction 3 Retrograde, slow: 16 days; degrees — (43)〉 (14)〉 Retrograde, swift: 33 days, 2 degrees (35)〉 (60)〉 Retrograde, swift: 33 days, 2 degrees (35)〉 (60)〉
127
退
Retrograde, slow: 16 days; degrees — (43)〉 (14)〉 Latter station: 37 days fraction 3 Prograde, slow: 19 days; degrees — (63)〉 (35)〉 Prograde, swift: 65 days, 6 degrees (38)〉 3 (51)〉
128
Evening hiding: 19 days, 2 degrees fraction 7 1 (14)〉 ◎ Venus cycle rate: 4,204,143; remainder 96. Variation rate: 4,204,143; remainder 96.
129
Calendar rate: 2,629,750; remainder 56. Sidereal period: 583 days; remainder 6,543; fraction 96. Mid-cycle: 182 days; remainder 4,475; fraction 28. Segment | Days | Degrees | Calendar
130
Evening appearance: 42 days, 53 degrees (40)〉 51 (17)〉
131
Prograde, swift: 96 days, 121 degrees (57)〉 116 (39)〉 Secondary swift: 73 days, 80 degrees (37)〉 77 fraction 2 Secondary slow: 33 days, 34 degrees fraction 1 32 (40)〉
132
退
Prograde, slow: 24 days, 11 degrees (61)〉 11 (24)〉 Prior station: 6 days (69)〉 Retrograde, slow: 4 days, 1 degree (22)〉 (31)〉
133
退
Retrograde, swift: 6 days, 3 degrees (65)〉 1 (22)〉 Evening hiding: 7 days, 4 degrees (40)〉 1 (37)〉 Morning appearance: 7 days, 4 degrees (40)〉 1 (37)〉
134
退 退
Retrograde, swift: 6 days, 3 degrees (65)〉 1 (22)〉 Retrograde, slow: 4 days, 1 degree (22)〉 (31)〉 Latter station: 6 days (69)〉
135
Prograde, slow: 24 days, 11 degrees (61)〉 11 (24)〉 Secondary slow: 33 days, 34 degrees fraction 1 32 (40)〉 Secondary swift: 73 days, 80 degrees (37)〉 77 fraction 2
136
Prograde, swift: 96 days, 121 degrees (57)〉 116 (39)〉
137
Morning concealment: 42 days, 53 degrees (40)〉 51 (17)〉 ◎ Mercury cycle rate: 834,335; remainder 52. Variation rate: 834,335; remainder 52.
138
Calendar rate: 2,629,760; remainder 44. Sidereal period: 115 days; remainder 6,335; fraction 52. Mid-cycle: 182 days; remainder 4,480; fraction 22. Segment | Days | Degrees | Calendar
139
Evening appearance: 17 days, 34 degrees fraction 1 29 (54)〉 Prograde, swift: 11 days, 18 degrees (24)〉 16 fraction 4 Prograde, slow: 16 days, 11 degrees (43)〉 10 (10)〉
140
Prior station: 2 days (68)〉 Evening concealment: 11 d, 6°, frac. 2; morning appearance: 11 d, 6°, frac. 2; latter station: 2 d (68)〉
141
Prograde, slow: 16 days, 11 degrees (43)〉 10 (10)〉 Prograde, swift: 11 days, 18 degrees (24)〉 16 fraction 4
142
Morning concealment: 17 days, 34 degrees fraction 1 29 (54)〉 ◎ Mean conjunction: day and central star
143
退 退
Set the qi accumulation and divide by the planet's cycle rate to obtain the number of complete cycles; the remainder is the accumulation before conjunction at celestial mid-qi. Subtract it from the annual rate to obtain the post-conjunction at celestial mid-qi in the preceding year. If the subtraction cannot be completed, add one annual rate and subtract again to obtain the post-conjunction two years earlier. Reduce each by the unification divisor to obtain days and degrees—the mean-conjunction mid-day and central star sought. Set the mid-day and add the segment mutation-days cumulatively to obtain each segment's mid-day. Set the central star and apply each segment's mutation-degrees, adding in direct motion and subtracting in retrograde, to obtain each segment's central star. Venus and Mercury evening concealment and morning appearance all use retrograde mutation.
144
滿
Set the variation rate. Multiply by the cycle count, remove multiples of the calendar rate, and convert the remainder to degrees by the unification divisor. If below mid-cycle, it is prior; if above, subtract the mid-cycle value to obtain the posterior portion—the mean-conjunction's entry into the epicycle sought. Add the segment mutation-calendar values cumulatively to obtain each segment's epicycle entry.
145
Prior-posterior fixed corrections
146
Set the epicycle parts, multiply by the degree's variation rate, divide by the canonical divisor, and apply the result to adjust the prior-posterior constants below—the value sought. ◎ Mean day and corrected star
147
宿宿
Set the mean day and central star and apply the prior-posterior corrections, adding when prior and subtracting when posterior; at stations use the prior segment's values. For Venus in direct concealment/appearance and the segments prior swift, secondary swift, posterior secondary slow, and secondary swift, and for Mercury in direct concealment/appearance with prior swift and posterior slow, reverse the rule (subtract when prior, add when posterior) to obtain each segment's mean day and corrected star. Set the corrected star, add the year's celestial mid-qi solar longitude on the ecliptic and name the lodge, to obtain each segment's terminal-day added-time lodge position.
148
Expansion and contraction corrections
149
Set the mean day; if it does not exceed the annual mid-cycle, it lies in the expansion phase; if above, subtract the annual mid-cycle; the remainder lies in contraction—the mean day's entry into the expansion-contraction epicycle. Set the epicycle parts. Multiply by the day's variation rate, divide by the canonical divisor, and adjust the expansion-contraction constant below to obtain the value sought.
150
Set the mean day and subtract in expansion or add in contraction according to the correction to obtain the corrected day. Add the year's celestial mid-qi and name the result to obtain each segment's terminal-day added-time date and hour. ◎ Entry into qi and solar terms
151
Set the corrected day, divide by the qi divisor, and count from the winter solstice to obtain the qi and day entered. ◎ Mean daily motion
152
Set the corrected day and subtract the prior segment's corrected day to obtain the day rate; subtract the prior segment's corrected star from the current corrected star to obtain the degree rate. Convert the degree rate, multiply by the canonical divisor, divide by the converted day rate, to obtain the mean daily motion. ◎ Initial and final daily motion
153
退
For a segment near concealment, average its mean motion with that of the concealment segment to obtain the near-concealment daily motion. Subtract from the mean motion; subtract the remainder again from the mean motion to obtain the far-concealment daily motion. Near-station segment: near-station daily motion is blank. Double the mean daily motion to obtain the far-station daily motion. For segments not near concealment or station, average the mean motions of the two adjacent direct-motion segments to obtain the last day of the prior segment and the first day of the next. Compare each with its segment's mean motion; if the mean motion is greater, add the mean motion; if less, subtract the mean motion—to obtain the first day of the prior segment and the last day of the posterior segment. For segments not near concealment or station in retrograde motion, take the slow segment's near-swift motion as the swift segment's near-slow motion; compare with the mean motion and add if the mean is greater or subtract if less—all yielding the far-slow daily motion.
154
宿
Initial motion: midnight lodge position
155
退宿宿
Set the canonical divisor and subtract the prior segment's terminal-day added-time parts; multiply the remainder by that day's motion and divide by the canonical divisor; add in direct motion or subtract in retrograde from the prior segment's terminal-day added-time lodge position to obtain this segment's initial dusk-after-midnight lodge position. ◎ Daily motion
156
退宿宿
Subtract the initial from the final daily motion to obtain the difference rate. Count the days from this segment's initial dusk-after-midnight to the next segment's initial dusk-after-midnight and divide to obtain the daily increment. Halve the daily increment and apply it to reduce the larger and increase the smaller to obtain the segment's corrected initial and final motion. Set the corrected initial motion and accumulate the daily increment, adding when the final motion is greater and subtracting when less, to obtain each day's motion. Apply each day's motion, adding in direct motion and subtracting in retrograde from the initial dusk-after-midnight position, to obtain the star's lodge at dusk after midnight for each day.
157
宿
Corrected day: dusk-after-midnight lodge position
158
退宿
Count the days from the segment's first day to the day sought and multiply by the segment's daily increment; add to or subtract from the first day's motion according to whether the final motion is greater or less to obtain that day's motion. Average with the first day's motion, multiply by the elapsed days, and add or subtract from the segment's initial dusk-after-midnight lodge position in direct or retrograde motion to obtain the result sought.
159
Qintian Calendar, procedure for pacing emergence and retraction—hou divisor: 5; remainder 524; fraction 45. Hexagram divisor: 6; remainder 629; fraction 34. Outer divisor: 3; remainder 314; fraction 67.
160
Intercalary divisor: 12; remainder 1,258; fraction 68. Solar-term surplus: 1,573; fraction 35.
161
New-moon void: 3,399; fraction 72. ◎ Climate chart — Winter Solstice (11th month, mid-month): earthworms coil; elk shed antlers; springs stir. Minor Cold (12th month, first node): wild geese turn north; magpies begin to nest; pheasants first call.
162
Major Cold (12th month, mid-month): hens begin brooding; birds of prey grow swift; ice hardens deep in the marshes. Start of Spring (1st month, first node): the east wind thaws the ice; dormant insects stir; fish rise beneath the ice. Rain Water (1st month, mid-month): otters offer fish; wild geese arrive; grass and trees put forth shoots.
163
Awakening of Insects (2nd month, first node): peaches blossom; orioles sing; hawks turn into cuckoos. Spring Equinox (2nd month, mid-month): swallows arrive; thunder sounds; lightning begins. Pure Brightness (3rd month, first node): paulownia blooms; field mice become quails; rainbows first appear.
164
滿
Grain Rain (3rd month, mid-month): duckweed sprouts; turtle-doves preen their feathers; hoopoes alight on mulberry trees. Start of Summer (4th month, first node): tree crickets chirp; earthworms emerge; gourds grow. Minor Fullness (4th month, mid-month): bitter herbs flourish; tender grasses wither; lesser heat draws near.
165
鹿
Grain in Ear (5th month, first node): praying mantises hatch; shrikes begin to call; mockingbirds fall silent. Summer Solstice (5th month, mid-month): deer shed antlers; cicadas begin to sing; pinellia sprouts. Minor Heat (6th month, first node): warm winds blow; crickets move to the walls; eagles learn to strike.
166
Major Heat (6th month, mid-month): rotten grass turns to fireflies; the earth grows damp in oppressive heat; heavy rains fall in season. Start of Autumn (7th month, first node): cool winds arrive; white dew descends; cold cicadas cry. End of Heat (7th month, mid-month): eagles offer birds; heaven and earth begin to harden; grain ripens.
167
White Dew (8th month, first node): wild geese arrive; swallows return; birds lay up provisions. Autumn Equinox (8th month, mid-month): thunder fades; hibernating creatures block their burrows; waters begin to shrink. Cold Dew (9th month, first node): geese come as guests; sparrows enter the water as clams; chrysanthemums bloom yellow.
168
Frost Descent (9th month, mid-month): jackals sacrifice game; plants yellow and shed their leaves; dormant insects all lie low. Start of Winter (10th month, first node): water begins to freeze; the earth begins to chill; pheasants enter the water as oysters.
169
Minor Snow (10th month, mid-month): rainbows vanish from sight; the qi of heaven rises and that of earth sinks; all closes into winter.
170
Major Snow (11th month, first node): the crossbill ceases to sing; tigers begin to mate; spring onions sprout. ◎ Hexagram-image chart.
171
Winter Solstice: 《Kan》, first six; duke 《Zhong Fu》; emperor 《Fu》; marquis 《Zhun》. (inner hexagrams)
172
Minor Cold: 《Kan》, nine in the second; marquis 《Zhun》. (outer hexagrams) Great officer 《Qian》; minister 《Kui》.
173
Major Cold: 《Kan》, six in the third; duke 《Sheng》; emperor 《Lin》; marquis 《Xiao Guo》. (inner hexagrams)
174
Start of Spring: 《Kan》, six in the fourth; marquis 《Xiao Guo》. (outer hexagrams) Great officer 《Meng》; minister 《Yi》.
175
Rain Water: 《Kan》, nine in the fifth; duke 《Jian》; emperor 《Tai》; marquis 《Xu》. (inner hexagrams)
176
Awakening of Insects: 《Kan》, top six; marquis 《Xu》. (outer hexagrams) Great officer 《Sui》; minister 《Jin》.
177
Spring Equinox: 《Zhen》, first nine; duke 《Xie》; emperor 《Da Zhuang》; marquis 《Yu》. (inner hexagrams)
178
Pure Brightness: 《Zhen》, six in the second; marquis 《Yu》. (outer hexagrams) Great officer 《Song》; minister 《Gu》.
179
Grain Rain: 《Zhen》, six in the third; duke 《Ge》; emperor 《》; marquis 《Lü》; inner.
180
Start of Summer: 《Zhen》, nine in the fourth; marquis 《Lü》. (outer hexagrams) Great officer 《Shi》; minister 《Bi》.
181
滿
Minor Fullness: 《Zhen》, six in the fifth; duke 《Xiao Xu》; emperor 《Qian》; marquis 《Da You》. (inner hexagrams)
182
Grain in Ear: 《Zhen》, top six; marquis 《Da You》. (outer hexagrams) Great officer 《Jia Ren》; minister 《Jing》.
183
Summer Solstice: 《Li》, first nine; duke 《Xian》; emperor 《Hou》; marquis 《Ding》; inner.
184
Minor Heat: 《Li》, six in the second; marquis 《Ding》. (outer hexagrams) Great officer 《Feng》; minister 《Huan》.
185
Major Heat: 《Li》, nine in the third; duke 《Lü》; emperor 《Dun》; marquis 《Heng》. (inner hexagrams)
186
Start of Autumn: 《Li》, nine in the fourth; marquis 《Heng》. (outer hexagrams) Great officer 《Jie》; minister 《Tong Ren》.
187
End of Heat: 《Li》, six in the fifth; duke 《Sun》; emperor 《Pi》; marquis 《Xun》. (inner hexagrams)
188
White Dew: 《Li》, top nine; marquis 《Xun》. (outer hexagrams) Great officer 《Cui》; minister 《Da Xu》.
189
Autumn Equinox: 《Dui》, first nine; duke 《Bi》; emperor 《Guan》; marquis 《Gui Mei》. (inner hexagrams)
190
Cold Dew: 《Dui》, nine in the second; marquis 《Gui Mei》. (outer hexagrams) Great officer 《Wu Wang》; minister 《Ming Yi》.
191
Frost Descent: 《Dui》, six in the third; duke 《Kun》; emperor 《Bo》; marquis 《Gen》. (inner hexagrams)
192
Start of Winter: 《Dui》, nine in the fourth; marquis 《Gen》. (outer hexagrams) Great officer 《Ji Ji》; minister 《Shi He》.
193
Minor Snow: 《Dui》, nine in the fifth; duke 《Da Guo》; emperor 《Kun》; marquis 《Wei Ji》. (inner hexagrams)
194
Major Snow: 《Dui》, top six; marquis 《Wei Ji》. (outer hexagrams) Great officer 《Jian》; minister 《Yi》. ◎ Seventy-two hou.
195
Set each at the mid-node of its solar term; that yields the first phenological hou. Add the hou divisor cumulatively to obtain each successive hou. ◎ The sixty-four hexagrams.
196
Set at the central qi; that is the duke hexagram. Add the hexagram divisor cumulatively to obtain each successive hexagram. From the marquis hexagram, add the outer divisor to obtain the outer hexagram. ◎ Governance of the Five Phases.
197
Fix the four establishment nodes and name them: that marks when Wood governs in spring, Fire in summer, Metal in autumn, and Water in winter. Fix the four seasonal nodes and add the intercalary divisor to each; that is when Earth governs. ◎ Submergence days (mo days).
198
滿
When the mid-node fraction is 5,626 seconds 65 or more, subtract the epoch divisor to obtain the submergence remainder. Multiply by the communicated qi divisor, divide by the qi surplus plus one, and convert remainders filling the epoch divisor into days; add the result to the qi and name the day to obtain the submergence day sought. ◎ Extinction days (extinguished days).
199
When the regular new-moon fraction falls at or below the new-moon void, that is the extinction remainder. multiply by the new-moon rate, divide by the new-moon void plus one, and convert remainders filling the epoch divisor into days; add the result to the new moon and name the day to obtain the extinction day sought.
200
使 使 使
At right, four chapters composed by Pu: the 《Qintian Calendar Classic》. The 《Old History》 lost its one chapter 《Pacing Emergence and Retraction》; of those remaining, three chapters are brief and incomplete, insufficient to serve as method. Pu's calendar had scarcely been handed down. I once asked Liu Xisou, Assistant in the Directorate of Authorship; he obtained the original classic for me, and only then did Pu's calendar stand complete. Xisou was a devoted scholar of history and letters, especially expert in astronomy and calendrics. He once told me: "Calendar-makers of earlier ages used different methods, and most of them were in error. Reaching Tang, Yixing first used heaven-and-earth central numbers to make the 《Dayan Calendar》, most precise and close. Later masters of calendrics all followed his method, merely copying fractions and adjusting figures. Pu, in his turn, was able to establish a school of his own. In Pu's method, solar motion discrepancies are summed into paired surplus-and-wane tables; lunar motion is divided into 248 slow-and-swift limits to track diminishing and waxing, to judge the moon's phases—so that new and full moons align correctly. He calibrated nine equatorial limits and revised their rates to pace the ecliptic, giving the sun's motion a fixed measure; he divided the ecliptic into eight nodes, distinguished inner from outer paths, and gauged the nine courses of the moon so that her motion runs in cycles and the two luminaries keep accord. He observed how celestial momentum rises and falls, examined whether orbits run oblique or true, and regulated eclipse discrepancy so that conjunctions grew exact. He measured the central gnomon at the Imperial Observatory to fix the day-lengths of the solstices, and the clepsydra matched the solar path. He computed planets' retrograde and direct motion, their hiding and station, giving slow and swift motion proper gradation so that the five planets kept in step. Yet he could not make the system broad, deep, and simple; he took what was quick and direct. In what he did best, not even a sage could set his work aside." Such, in sum, was Xisou's judgment, which readers may consult for themselves.
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