卷四·第 214–221 问 城市经纬度、日出方位与昼夜长短
城市的纬度与经度、经度的两种起点,经纬不同的两城有何差别,日出方位的幅度,以及昼夜为何随纬度与季节长短。
§214. What is the latitude of a town?
It is its shortest distance from the equinoctial line towards the north, because the towns are in this region. Facing it in the sky is a similar great-circle arc lying between the zenith and the equator, and the altitude of the north pole is equal to it; that is why the latitude is expressed by that altitude. The depression of the south pole, though it is equal to it as well, is hidden and not perceived.
翻译点开
§214. What is the latitude of a town?
第二百一十四问 何谓城市的纬度?
It is its shortest distance from the equinoctial line towards the north, because the towns are in this region. Facing it in the sky is a similar great-circle arc lying between the zenith and the equator, and the altitude of the north pole is equal to it; that is why the latitude is expressed by that altitude. The depression of the south pole, though it is equal to it as well, is hidden and not perceived.
它是城市向北离赤道线的最短距离,因为诸城都在这一区域。天上与它相对的,是天顶与天赤道之间一段与之相似的大圆弧,北极的高度与它相等;所以纬度就用这个高度来表示。南极的低落虽然也与它相等,但隐而不见,觉察不到。
大意与图解点开
🔎 大意:城市纬度是它向北离赤道线的最短距离,天上对应天顶到天赤道之弧,等于北极高度,所以以北极高度表示。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 纬度 | the latitude of a town | 离赤道线向北的距离 |
| 北极的高度 | the altitude of the north pole | 北极高出地平之弧 |
| 天顶 | zenith | 头顶正上方 |
| 低落 | depression | 低于地平之弧 |
🧭 图解与讲解
城市的纬度,是它向北离赤道线的最短距离。比鲁尼只说“向北”,因为上一章说过,有人居住之地全在北方。地上的这段距离,在天上有一段相似的弧与之相对:从天顶到天赤道的那段子午圈(图一)。
〔图〕城市的纬度等于天顶到天赤道之弧,也等于北极高出地平之弧
这段弧又恰好等于北极高出地平的弧。道理很简单:天顶与地平相距九十度,天赤道与北极也相距九十度,两段各去掉中间共有的一段,剩下的自然相等。所以要知道一个城市的纬度,只要测北极(实际上测北极附近的星或正午的日影)有多高。南极低于地平同样多,但看不见,无从量起。
纬度是占星计算里最常用的数之一:同一时刻,同样的天象,纬度不同,上升点、宫位的划分、星座的上升时间、昼夜的长短就都不同。后面几问讲的正是纬度带来的这些差别。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 纬度 | the latitude of a town | 离赤道线向北的距离 |
| 北极的高度 | the altitude of the north pole | 北极高出地平之弧 |
| 天顶 | zenith | 头顶正上方 |
| 低落 | depression | 低于地平之弧 |
🧭 图解与讲解
城市的纬度,是它向北离赤道线的最短距离。比鲁尼只说“向北”,因为上一章说过,有人居住之地全在北方。地上的这段距离,在天上有一段相似的弧与之相对:从天顶到天赤道的那段子午圈(图一)。
这段弧又恰好等于北极高出地平的弧。道理很简单:天顶与地平相距九十度,天赤道与北极也相距九十度,两段各去掉中间共有的一段,剩下的自然相等。所以要知道一个城市的纬度,只要测北极(实际上测北极附近的星或正午的日影)有多高。南极低于地平同样多,但看不见,无从量起。
纬度是占星计算里最常用的数之一:同一时刻,同样的天象,纬度不同,上升点、宫位的划分、星座的上升时间、昼夜的长短就都不同。后面几问讲的正是纬度带来的这些差别。
§215. What is the longitude of a town?
It is its distance from the farthest end of habitation, whether taken on the equator, or on the equinoctial line, or on the line of the towns parallel to them; for the similarity between them makes one stand in place of the other. Since what we use of this art is derived from the views of the Greeks, and they began longitude from the nearer of the two ends of habitation to them, which is the western one, the longitude of a town is therefore its distance from the west. But on this end there is disagreement among them: some of them begin longitude from the shore of the western Ocean, and some from six islands lying far out in the sea, about 200 farsakhs, called the Islands of Happiness and the Eternal Islands (al-Khālidāt), which are opposite the west. So two kinds of longitude may be found in the books for one town, with 10 degrees between them, and to distinguish them requires discernment and practice.
§216. What is called 'between the two longitudes'?
It is the difference between the longitudes of the two towns, and it is equal to the times between their two meridians, whether on the equator or on each of the daily orbits of the two towns or on others.

翻译点开
§215. What is the longitude of a town?
第二百一十五问 何谓城市的经度?
It is its distance from the farthest end of habitation, whether taken on the equator, or on the equinoctial line, or on the line of the towns parallel to them; for the similarity between them makes one stand in place of the other. Since what we use of this art is derived from the views of the Greeks, and they began longitude from the nearer of the two ends of habitation to them, which is the western one, the longitude of a town is therefore its distance from the west. But on this end there is disagreement among them: some of them begin longitude from the shore of the western Ocean, and some from six islands lying far out in the sea, about 200 farsakhs, called the Islands of Happiness and the Eternal Islands (al-Khālidāt), which are opposite the west. So two kinds of longitude may be found in the books for one town, with 10 degrees between them, and to distinguish them requires discernment and practice.
它是城市离有人居住之地最远一端的距离,无论是在天赤道上量、在赤道线上量,还是在城市所在的、与二者平行的那条线上量;因为三者相似,所以可以互相代替。由于我们在这门学问中所用的,是从希腊人的见解中得来的,而他们是从有人居住之地两端中离他们较近的一端,也就是西端,开始起算经度的,所以城市的经度就是它离西方的距离。但在这一端上,他们之间有分歧:有些人从西方大洋的岸边起算经度,有些人则从远在海中约二百法尔萨赫的六座岛屿起算,这些岛称为幸福群岛和永生群岛,正对着西方。所以书中对同一座城市可能有两种经度,相差十度,要分辨它们,需要眼力和练习。
§216. What is called 'between the two longitudes'?
第二百一十六问 何谓“两经之间”?
It is the difference between the longitudes of the two towns, and it is equal to the times between their two meridians, whether on the equator or on each of the daily orbits of the two towns or on others.
它是两座城市经度之差,等于它们两条子午线之间的时度,无论是在天赤道上量、在两城各自的日周圈上量,还是在别的圈上量。
大意与图解点开
🔎 大意:经度是城市离人居之地西端的距离,或自西海岸、或自海中的幸福群岛起算,相差十度;两城经度之差即两子午线间的时度。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 经度 | the longitude of a town | 离西端的距离 |
| 幸福群岛 | the Islands of Happiness | 经度的另一起点 |
| 永生群岛 | the Eternal Islands (al-Khālidāt) | 幸福群岛的别名 |
| 两经之间 | 'between the two longitudes' | 两城经度之差 |
| 时度 | times | 在天赤道上量的度 |
🧭 图解与讲解
经度从哪里量起?比鲁尼说,这门学问承自希腊人,而有人居住之地的两端中,西端离希腊人较近,所以经度从西端往东量。“在天赤道上量,在赤道线上量,还是在城市所在的平行线上量”,都是相似的弧,度数相同,可以互相代替。
| 经度的起点 | 所在 | 后果 |
|---|---|---|
| 西方大洋的岸边 | 有人居住之地的西端 | 一派由此起算 |
| 幸福群岛(永生群岛) | 海中约二百法尔萨赫外的六座岛,正对西方 | 另一派由此起算 |
| 两派之差 | — | 同一城市书中可有两种经度,相差十度,须分辨 |
〔图〕两城经度之差就是两条子午线之间的时度,东城的正午先到
西端本身却有两说(表一):一说从西方大洋的岸边起算;一说从海中约二百法尔萨赫外的六座岛起算,这些岛称为“幸福群岛”或“永生群岛”(al-Khālidāt)。两种起点相差十度,所以同一座城,在不同的书里经度可能差十度。比鲁尼提醒读者,用别人的经度表之前,要先弄清它从哪里起算,这需要“眼力和练习”。
“两经之间”是两城经度之差,等于两城子午线之间的时度(图二)。天一日转一周,三百六十时度合二十四个等时,每十五时度合一小时。所以经度差十五度的两城,东边那座的正午比西边早一小时。这正是占星里“换地换时”的根据:别处的星历要拿来本地用,先要按经度差把时刻换算过来。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 经度 | the longitude of a town | 离西端的距离 |
| 幸福群岛 | the Islands of Happiness | 经度的另一起点 |
| 永生群岛 | the Eternal Islands (al-Khālidāt) | 幸福群岛的别名 |
| 两经之间 | 'between the two longitudes' | 两城经度之差 |
| 时度 | times | 在天赤道上量的度 |
🧭 图解与讲解
经度从哪里量起?比鲁尼说,这门学问承自希腊人,而有人居住之地的两端中,西端离希腊人较近,所以经度从西端往东量。“在天赤道上量,在赤道线上量,还是在城市所在的平行线上量”,都是相似的弧,度数相同,可以互相代替。
| 经度的起点 | 所在 | 后果 |
|---|---|---|
| 西方大洋的岸边 | 有人居住之地的西端 | 一派由此起算 |
| 幸福群岛(永生群岛) | 海中约二百法尔萨赫外的六座岛,正对西方 | 另一派由此起算 |
| 两派之差 | — | 同一城市书中可有两种经度,相差十度,须分辨 |
西端本身却有两说(表一):一说从西方大洋的岸边起算;一说从海中约二百法尔萨赫外的六座岛起算,这些岛称为“幸福群岛”或“永生群岛”(al-Khālidāt)。两种起点相差十度,所以同一座城,在不同的书里经度可能差十度。比鲁尼提醒读者,用别人的经度表之前,要先弄清它从哪里起算,这需要“眼力和练习”。
“两经之间”是两城经度之差,等于两城子午线之间的时度(图二)。天一日转一周,三百六十时度合二十四个等时,每十五时度合一小时。所以经度差十五度的两城,东边那座的正午比西边早一小时。这正是占星里“换地换时”的根据:别处的星历要拿来本地用,先要按经度差把时刻换算过来。
§217. What follows from the difference in longitude of two towns when their latitudes are equal?
Nothing follows for them from that except the difference in rising and setting: the beginning of daytime or of night in the eastern of the two, which is the one of greater longitude, always comes before it comes in the western one by the amount between their longitudes; and midday and midnight are in them by the same reckoning. The nature of the air does not differ between them except through some accident affecting one of them from a difference of position with respect to seas, mountains, sands, lowland or highland; otherwise the two are alike.
§218. What follows from the difference in latitude of two towns when their longitudes are equal?
Midday or midnight comes to both of them at one time, and so does the rising and the setting of the Sun when it is at the beginning of Aries and of Libra; and in the same way the rising and setting of every star that is on the equator. But when the Sun or the star is not on the equator itself but has moved away from it to the south, its rising on the town of smaller latitude comes before its rising on the town of greater latitude, and its setting on the town of smaller latitude after its setting on the town of greater latitude. If the Sun or the star is north of the equator, the matter is the reverse of what we have said: I mean, its rising on the town of smaller latitude comes after its rising on the town of greater latitude, and its setting on the town of smaller latitude before its setting on the town of greater latitude. The 'before' and 'after' in this have no regular amount. Further, the lengths of one and the same daytime and of its night differ in the two, when they are unequal; the amplitude of the risings, the altitude at midday and its shadow differ; the stars that are always visible and those always hidden differ; and the one of greater latitude is colder in air, unless some circumstance of position arises in them, so that the preponderance goes to the one of greater latitude over the other in heat of air [text uncertain]; as with Ghazna among the cold lands and Baghdad among the hot lands, whose latitudes are equal.
§219. What follows from a difference in both longitudes and latitudes of two towns together?
In them there occurs all that we have mentioned of the two kinds of difference, composed of the two taken singly; and the rising of a star in one and its setting in the other do not coincide in them except when it is on one of the two points at which their horizons intersect.
翻译点开
§217. What follows from the difference in longitude of two towns when their latitudes are equal?
第二百一十七问 两座城市纬度相等而经度不同,会生出什么来?
Nothing follows for them from that except the difference in rising and setting: the beginning of daytime or of night in the eastern of the two, which is the one of greater longitude, always comes before it comes in the western one by the amount between their longitudes; and midday and midnight are in them by the same reckoning. The nature of the air does not differ between them except through some accident affecting one of them from a difference of position with respect to seas, mountains, sands, lowland or highland; otherwise the two are alike.
由此对它们生出的,只有升起与落下的不同:白昼或黑夜的开始,在两城中偏东的那一座,也就是经度较大的那一座,总是比在偏西的那一座来得早,早的量就是两城的经度之差;正午和子夜在两城也照此计算。两城空气的性质并无不同,除非其中一城因在海、山、沙地、低地或高地方面位置不同,而受到某种偶然的影响;否则二者是一样的。
§218. What follows from the difference in latitude of two towns when their longitudes are equal?
第二百一十八问 两座城市经度相等而纬度不同,会生出什么来?
Midday or midnight comes to both of them at one time, and so does the rising and the setting of the Sun when it is at the beginning of Aries and of Libra; and in the same way the rising and setting of every star that is on the equator. But when the Sun or the star is not on the equator itself but has moved away from it to the south, its rising on the town of smaller latitude comes before its rising on the town of greater latitude, and its setting on the town of smaller latitude after its setting on the town of greater latitude. If the Sun or the star is north of the equator, the matter is the reverse of what we have said: I mean, its rising on the town of smaller latitude comes after its rising on the town of greater latitude, and its setting on the town of smaller latitude before its setting on the town of greater latitude. The 'before' and 'after' in this have no regular amount. Further, the lengths of one and the same daytime and of its night differ in the two, when they are unequal; the amplitude of the risings, the altitude at midday and its shadow differ; the stars that are always visible and those always hidden differ; and the one of greater latitude is colder in air, unless some circumstance of position arises in them, so that the preponderance goes to the one of greater latitude over the other in heat of air [text uncertain]; as with Ghazna among the cold lands and Baghdad among the hot lands, whose latitudes are equal.
正午或子夜同时到达两城,太阳在白羊座起点和天秤座起点时的升起与落下也是同时的;同样,凡在天赤道上的星,其升落也同时。但当太阳或星不在天赤道本身,而是离开它向南时,它在纬度较小之城的升起早于在纬度较大之城的升起,它在纬度较小之城的落下晚于在纬度较大之城的落下。若太阳或星在天赤道以北,情形就与我们所说的相反:我是说,它在纬度较小之城的升起晚于在纬度较大之城的升起,它在纬度较小之城的落下早于在纬度较大之城的落下。这里的“早”与“晚”没有固定的量。此外,在昼夜不等的时候,同一个白昼及其黑夜的长度在两城中也不同;日出方位的幅度、正午的高度及其影长都不同;恒显之星和恒隐之星也不同;纬度较大的一城空气较冷,除非两城出现某种位置上的情况,使纬度较大的一城在空气的热度上反而胜过另一城〔原文疑有讹误〕;例如寒冷之地中的伽色尼与炎热之地中的巴格达,二者纬度相等。
§219. What follows from a difference in both longitudes and latitudes of two towns together?
第二百一十九问 两座城市经度和纬度都不同,会生出什么来?
In them there occurs all that we have mentioned of the two kinds of difference, composed of the two taken singly; and the rising of a star in one and its setting in the other do not coincide in them except when it is on one of the two points at which their horizons intersect.
在它们之中,会出现我们所说两类差异的全部情形,由二者各自单独的情形合成;而且一颗星在其中一城的升起与在另一城的落下,除非它恰好在两城地平相交的两点之一上,否则不会同时发生。
大意与图解点开
🔎 大意:纬同经异,只差升落时刻;经同纬异,正午同时而昼夜长短、日出幅度、正午高度、恒显恒隐之星、冷暖都不同;两者都异则兼有之。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 偏东 | the eastern of the two | 经度较大的一城 |
| 恒显之星 | the stars always visible | 绕极不落之星 |
| 正午的高度 | the altitude at midday | 中天时的高度 |
| 伽色尼 | Ghazna | 比鲁尼所居之城 |
🧭 图解与讲解
这三问把经度、纬度的作用分开来看(表一)。纬度相同、经度不同的两城,天象完全一样,只是时刻有先后:东城(经度较大)的日出、正午、日落、子夜,都比西城早,早的量就是经度之差。气候也一样,除非海、山、沙地、高低这些地势造成偶然的差别。
| 两城的情形 | 相同的 | 不同的 |
|---|---|---|
| 纬度同,经度异 | 空气性质(除非地势有偶然影响) | 升落、正午、子夜的时刻:东城先到,先的量等于经度之差 |
| 经度同,纬度异 | 正午、子夜同时;太阳在春秋分点、以及天赤道上的星,升落同时 | 赤道以南之星:低纬之城升得早、落得晚;以北之星相反,早晚没有定量。另有昼夜长短、日出幅度、正午高度与影长、恒显恒隐之星、冷暖 |
| 经纬都异 | — | 兼有上两类差异;一星此升彼落,只有在两城地平相交的两点上才同时 |
〔图〕纬度相同,冷暖也可以相反:地势能压过纬度
经度相同、纬度不同的两城,正午和子夜同时;太阳在春分、秋分时,以及一切在天赤道上的星,升落也同时。但赤道以南的星,在低纬之城升得早、落得晚;赤道以北的星正相反。这“早晚”没有固定的量,因为它随星的赤纬和两城的纬度而变。此外,两城的昼夜长短、日出方位的幅度、正午的高度与日影、哪些星永远不落、哪些永远不出,也都不同;一般说来,纬度较高的城较冷。
这里抄本有一处讹误,大意是地势可以使纬度较高之城反而较暖。比鲁尼举的例子是伽色尼(Ghazna)与巴格达:两城纬度相等,伽色尼却是有名的冷地,巴格达是有名的热地(图二)。伽色尼是比鲁尼写这本书时所在的城市,他是以亲身所知举例。
经纬都不同的两城,兼有上面两类差别。比鲁尼又补一句:一颗星在甲城升起、同时在乙城落下,只有当它恰在两城地平相交的点上才可能。对占星来说,这几问说明为什么同一时刻的星盘必须按出生地或问事地的经纬度起:经度决定时刻,纬度决定上升点与宫位。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 偏东 | the eastern of the two | 经度较大的一城 |
| 恒显之星 | the stars always visible | 绕极不落之星 |
| 正午的高度 | the altitude at midday | 中天时的高度 |
| 伽色尼 | Ghazna | 比鲁尼所居之城 |
🧭 图解与讲解
这三问把经度、纬度的作用分开来看(表一)。纬度相同、经度不同的两城,天象完全一样,只是时刻有先后:东城(经度较大)的日出、正午、日落、子夜,都比西城早,早的量就是经度之差。气候也一样,除非海、山、沙地、高低这些地势造成偶然的差别。
| 两城的情形 | 相同的 | 不同的 |
|---|---|---|
| 纬度同,经度异 | 空气性质(除非地势有偶然影响) | 升落、正午、子夜的时刻:东城先到,先的量等于经度之差 |
| 经度同,纬度异 | 正午、子夜同时;太阳在春秋分点、以及天赤道上的星,升落同时 | 赤道以南之星:低纬之城升得早、落得晚;以北之星相反,早晚没有定量。另有昼夜长短、日出幅度、正午高度与影长、恒显恒隐之星、冷暖 |
| 经纬都异 | — | 兼有上两类差异;一星此升彼落,只有在两城地平相交的两点上才同时 |
经度相同、纬度不同的两城,正午和子夜同时;太阳在春分、秋分时,以及一切在天赤道上的星,升落也同时。但赤道以南的星,在低纬之城升得早、落得晚;赤道以北的星正相反。这“早晚”没有固定的量,因为它随星的赤纬和两城的纬度而变。此外,两城的昼夜长短、日出方位的幅度、正午的高度与日影、哪些星永远不落、哪些永远不出,也都不同;一般说来,纬度较高的城较冷。
这里抄本有一处讹误,大意是地势可以使纬度较高之城反而较暖。比鲁尼举的例子是伽色尼(Ghazna)与巴格达:两城纬度相等,伽色尼却是有名的冷地,巴格达是有名的热地(图二)。伽色尼是比鲁尼写这本书时所在的城市,他是以亲身所知举例。
经纬都不同的两城,兼有上面两类差别。比鲁尼又补一句:一颗星在甲城升起、同时在乙城落下,只有当它恰在两城地平相交的点上才可能。对占星来说,这几问说明为什么同一时刻的星盘必须按出生地或问事地的经纬度起:经度决定时刻,纬度决定上升点与宫位。
§220. What is the amplitude of the rising?
When the Sun is at the beginning of Aries and of Libra, it rises and sets in line with the equinoctial line which we derived by means of the Indian circle. When it inclines to the north, its rising and setting are in line with two points on the northern half of the horizon, which are the ends of a line parallel to the equinoctial line; and they keep getting farther from it until the Sun reaches the beginning of Cancer, and then the two points of its rising and setting are called the summer rising and its setting. Likewise, when it inclines towards the south, its rising and setting are in line with two points on the southern half of the horizon, which keep getting farther from the equinoctial line until the Sun reaches the beginning of Capricorn, and then the two points of its rising and setting are called the winter rising and its setting. The amplitude of the rising, then, is what lies between the equinoctial line and its place of rising. On the equinoctial line it is equal to the declination, but in towns that have latitudes the amplitude of the rising or of the setting exceeds the declination, and the greater the latitude, the greater the amplitude. This is the figure of it.

翻译点开
§220. What is the amplitude of the rising?
第二百二十问 何谓日出方位的幅度?
When the Sun is at the beginning of Aries and of Libra, it rises and sets in line with the equinoctial line which we derived by means of the Indian circle. When it inclines to the north, its rising and setting are in line with two points on the northern half of the horizon, which are the ends of a line parallel to the equinoctial line; and they keep getting farther from it until the Sun reaches the beginning of Cancer, and then the two points of its rising and setting are called the summer rising and its setting. Likewise, when it inclines towards the south, its rising and setting are in line with two points on the southern half of the horizon, which keep getting farther from the equinoctial line until the Sun reaches the beginning of Capricorn, and then the two points of its rising and setting are called the winter rising and its setting. The amplitude of the rising, then, is what lies between the equinoctial line and its place of rising. On the equinoctial line it is equal to the declination, but in towns that have latitudes the amplitude of the rising or of the setting exceeds the declination, and the greater the latitude, the greater the amplitude. This is the figure of it.
太阳在白羊座起点和天秤座起点时,正对着我们用印度圆求出的春秋分线升起和落下。当它向北偏时,它的升起和落下正对着地平北半上的两点,这两点是一条与春秋分线平行之线的两端;它们离春秋分线越来越远,直到太阳到达巨蟹座起点,这时它升起和落下的两点就称为夏季的日出处和夏季的日落处。同样,当它向南偏时,它的升起和落下正对着地平南半上的两点,这两点离春秋分线越来越远,直到太阳到达摩羯座起点,这时它升起和落下的两点就称为冬季的日出处和冬季的日落处。所以,日出方位的幅度就是春秋分线与它的升起之处之间的那段。在赤道线上,它等于赤纬;但在有纬度的城市里,日出或日落方位的幅度大于赤纬,纬度越大,幅度越大。这是它的图。
大意与图解点开
🔎 大意:春秋分日出正东;太阳北行则出没点移向北,到巨蟹座最远,南行反之。东西线到日出点的弧即幅度,纬度越大幅度越大。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 日出方位的幅度 | the amplitude of the rising | 日出点离正东之弧 |
| 春秋分线 | the equinoctial line (khaṭṭ al-iʿtidāl) | 地上的东西线 |
| 印度圆 | the Indian circle | 以表影定东西的方法 |
| 夏季的日出处 | the summer rising | 巨蟹座起点时的日出点 |
| 赤纬 | declination | 离天赤道的南北距离 |
🧭 图解与讲解
这一问的“春秋分线”,是地面上的东西线,前面讲过用“印度圆”(立表测影)求出。太阳在春分、秋分时,正对着这条线的两端升起和落下,也就是正东、正西(图一)。原书的图把地平画成一个圆,南在上、北在下,东在左、西在右,本站照此重画。
〔图〕日出方位的幅度:东西线到日出点之弧,夏至、冬至时最大
| 纬度 | 0°(赤道线上) | 20° | 30° | 40° | 50° |
|---|---|---|---|---|---|
| 夏至、冬至日出幅度 | 23.6° | 25.2° | 27.5° | 31.5° | 38.5° |
太阳走到北方星座时,出没点移到地平的北半,两点连线始终与东西线平行;到巨蟹座起点(夏至)最远,这两点称为“夏季的日出处”“夏季的日落处”。南行则移到南半,到摩羯座起点(冬至)最远,称为冬季的日出处、日落处。东西线与日出点之间的弧,就是“日出方位的幅度”。
幅度与纬度有关(表二):在赤道线上,幅度正好等于太阳的赤纬;离赤道越远,地平越斜,同样的赤纬造成的幅度就越大。表二是讲解按今法算的示意数,以夏至为例:赤道上约二十三度半,纬度三十度约二十七度半,五十度时已近三十八度半。
日出方位在古代有很实际的用处:定方向、建礼拜的朝向、安排田事。占星里,太阳、月亮与诸星从地平哪一点升起,也关系到它们在本地的上升与可见与否,下一问的昼夜长短,正是同一个道理的另一面。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 日出方位的幅度 | the amplitude of the rising | 日出点离正东之弧 |
| 春秋分线 | the equinoctial line (khaṭṭ al-iʿtidāl) | 地上的东西线 |
| 印度圆 | the Indian circle | 以表影定东西的方法 |
| 夏季的日出处 | the summer rising | 巨蟹座起点时的日出点 |
| 赤纬 | declination | 离天赤道的南北距离 |
🧭 图解与讲解
这一问的“春秋分线”,是地面上的东西线,前面讲过用“印度圆”(立表测影)求出。太阳在春分、秋分时,正对着这条线的两端升起和落下,也就是正东、正西(图一)。原书的图把地平画成一个圆,南在上、北在下,东在左、西在右,本站照此重画。
| 纬度 | 0°(赤道线上) | 20° | 30° | 40° | 50° |
|---|---|---|---|---|---|
| 夏至、冬至日出幅度 | 23.6° | 25.2° | 27.5° | 31.5° | 38.5° |
太阳走到北方星座时,出没点移到地平的北半,两点连线始终与东西线平行;到巨蟹座起点(夏至)最远,这两点称为“夏季的日出处”“夏季的日落处”。南行则移到南半,到摩羯座起点(冬至)最远,称为冬季的日出处、日落处。东西线与日出点之间的弧,就是“日出方位的幅度”。
幅度与纬度有关(表二):在赤道线上,幅度正好等于太阳的赤纬;离赤道越远,地平越斜,同样的赤纬造成的幅度就越大。表二是讲解按今法算的示意数,以夏至为例:赤道上约二十三度半,纬度三十度约二十七度半,五十度时已近三十八度半。
日出方位在古代有很实际的用处:定方向、建礼拜的朝向、安排田事。占星里,太阳、月亮与诸星从地平哪一点升起,也关系到它们在本地的上升与可见与否,下一问的昼夜长短,正是同一个道理的另一面。
§221. How do daytime and night lengthen in the towns?
The Sun turns either on the equator or on an orbit parallel to it, and the pole of all of them is the pole of the universe. When the horizon passes through the pole, and that is on the equinoctial line, it cuts the equator and the orbits parallel to it in halves, so that what is above the horizon of them equals what is below it; and so night and daytime are always equal there. When a town moves away from the equinoctial line, so that it has a latitude in the north and the pole is raised by its amount, the horizon does not pass through the pole and does not cut any circle in halves except the equator, because the two are both great circles; and so night and daytime are equal in all dwelling places when the Sun enters the beginning of Aries and of Libra, for these two are on the equator. As for the other orbits, the horizon cuts them in such an arrangement that what is above the horizon of the northern ones is greater than what is below it; and so in the northern signs the daytime lengthens and the night shortens. As for the southern ones, what of them is above the horizon is smaller than what is below it; and so in the southern signs the daytime shortens and the night lengthens. When the distance of two orbits from the equator is the same, one of them in the north and the other in the south, the increase and decrease of daytime and night in them are the same, and they are reciprocal in daytime and night: I mean that the daytime of one of them is equal to the night of the other.
翻译点开
§221. How do daytime and night lengthen in the towns?
第二百二十一问 城市里的白昼与黑夜怎样变长?
The Sun turns either on the equator or on an orbit parallel to it, and the pole of all of them is the pole of the universe. When the horizon passes through the pole, and that is on the equinoctial line, it cuts the equator and the orbits parallel to it in halves, so that what is above the horizon of them equals what is below it; and so night and daytime are always equal there. When a town moves away from the equinoctial line, so that it has a latitude in the north and the pole is raised by its amount, the horizon does not pass through the pole and does not cut any circle in halves except the equator, because the two are both great circles; and so night and daytime are equal in all dwelling places when the Sun enters the beginning of Aries and of Libra, for these two are on the equator. As for the other orbits, the horizon cuts them in such an arrangement that what is above the horizon of the northern ones is greater than what is below it; and so in the northern signs the daytime lengthens and the night shortens. As for the southern ones, what of them is above the horizon is smaller than what is below it; and so in the southern signs the daytime shortens and the night lengthens. When the distance of two orbits from the equator is the same, one of them in the north and the other in the south, the increase and decrease of daytime and night in them are the same, and they are reciprocal in daytime and night: I mean that the daytime of one of them is equal to the night of the other.
太阳或在天赤道上转,或在与之平行的轨道上转,这些轨道全都以宇宙之极为极。当地平通过极时,那是在赤道线上,它就把天赤道和与之平行的诸轨道都切成两半,于是诸轨道在地平以上的部分等于地平以下的部分;所以那里昼夜总是相等。当一座城市离开赤道线,在北方有了纬度,极按纬度的大小升高时,地平就不再通过极,除了天赤道,它不把任何圈切成两半,因为二者都是大圆;所以当太阳进入白羊座起点和天秤座起点时,一切住处昼夜都相等,因为这两点在天赤道上。至于其余的轨道,地平切它们的方式是:北方诸轨道在地平以上的部分大于地平以下的部分;所以在北方诸星座中,白昼变长,黑夜变短。至于南方诸轨道,在地平以上的部分小于地平以下的部分;所以在南方诸星座中,白昼变短,黑夜变长。当两条轨道离天赤道的距离相同,一条在北、一条在南时,它们的昼夜增减是相同的,而且在昼夜上互相对调:我是说,其中一条的白昼等于另一条的黑夜。
大意与图解点开
🔎 大意:赤道线上地平过两极,诸轨道都被平分,昼夜常等;有纬度处只有天赤道被平分,北方星座昼长夜短,南方相反,南北对称者昼夜互换。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 轨道 | orbit | 太阳每日所绕之圈 |
| 宇宙之极 | the pole of the universe | 天北极 |
| 大圆 | great circle | 圆心即球心的圆 |
| 北方诸星座 | the northern signs | 白羊至处女 |
🧭 图解与讲解
昼夜长短,归根到底是地平怎样切太阳每天绕行的那个圈。太阳每日沿着天赤道或与它平行的小圈(日周圈)转一周,这些圈都以天极为极。在赤道线上,地平正好通过两极,所以每一个这样的圈都被地平平分,上一半是昼,下一半是夜,终年昼夜相等。
〔图〕有纬度的地方,地平只把天赤道切成两半;北方轨道在地平上的多,昼长夜短,南方相反
| 纬度 | 0° | 20° | 30° | 40° | 50° |
|---|---|---|---|---|---|
| 太阳在巨蟹座起点:昼 | 12 时 | 13 时 13 分 | 13 时 57 分 | 14 时 52 分 | 16 时 11 分 |
| 同日:夜 | 12 时 | 10 时 47 分 | 10 时 3 分 | 9 时 8 分 | 7 时 49 分 |
| 太阳在摩羯座起点:昼 | 12 时 | 10 时 47 分 | 10 时 3 分 | 9 时 8 分 | 7 时 49 分 |
城市有了北纬,北极就升高同样的度数,地平不再通过天极。这时地平只能平分天赤道,因为两者都是大圆,大圆与大圆必互相平分;其余平行小圈都被切得不等(图一)。所以春分、秋分太阳在天赤道上时,各地昼夜都相等;太阳在北方星座,日周圈在地平以上的部分较多,昼长夜短;在南方星座则反过来。
最后一句很精巧:赤纬相同、一南一北的两个日周圈,昼夜正好对调,一个的白昼等于另一个的黑夜。表二是讲解按今法算的示意:纬度三十度时,夏至昼长约十三时五十七分,冬至的夜也正是这个长度。纬度越高,差距越大。
这一问是占星计算的一块基石。卷三讲过不等时(每段白昼分为十二);昼弧与夜弧的长短,直接决定不等时的长短、星座的上升时间,以及按半弧来分宫位的方法。下一章接着讲昼弧及其增减,比鲁尼在这里先把原理讲清。
📖 术语
| 术语 | 英文原词 | 意思 |
|---|---|---|
| 轨道 | orbit | 太阳每日所绕之圈 |
| 宇宙之极 | the pole of the universe | 天北极 |
| 大圆 | great circle | 圆心即球心的圆 |
| 北方诸星座 | the northern signs | 白羊至处女 |
🧭 图解与讲解
昼夜长短,归根到底是地平怎样切太阳每天绕行的那个圈。太阳每日沿着天赤道或与它平行的小圈(日周圈)转一周,这些圈都以天极为极。在赤道线上,地平正好通过两极,所以每一个这样的圈都被地平平分,上一半是昼,下一半是夜,终年昼夜相等。
| 纬度 | 0° | 20° | 30° | 40° | 50° |
|---|---|---|---|---|---|
| 太阳在巨蟹座起点:昼 | 12 时 | 13 时 13 分 | 13 时 57 分 | 14 时 52 分 | 16 时 11 分 |
| 同日:夜 | 12 时 | 10 时 47 分 | 10 时 3 分 | 9 时 8 分 | 7 时 49 分 |
| 太阳在摩羯座起点:昼 | 12 时 | 10 时 47 分 | 10 时 3 分 | 9 时 8 分 | 7 时 49 分 |
城市有了北纬,北极就升高同样的度数,地平不再通过天极。这时地平只能平分天赤道,因为两者都是大圆,大圆与大圆必互相平分;其余平行小圈都被切得不等(图一)。所以春分、秋分太阳在天赤道上时,各地昼夜都相等;太阳在北方星座,日周圈在地平以上的部分较多,昼长夜短;在南方星座则反过来。
最后一句很精巧:赤纬相同、一南一北的两个日周圈,昼夜正好对调,一个的白昼等于另一个的黑夜。表二是讲解按今法算的示意:纬度三十度时,夏至昼长约十三时五十七分,冬至的夜也正是这个长度。纬度越高,差距越大。
这一问是占星计算的一块基石。卷三讲过不等时(每段白昼分为十二);昼弧与夜弧的长短,直接决定不等时的长短、星座的上升时间,以及按半弧来分宫位的方法。下一章接着讲昼弧及其增减,比鲁尼在这里先把原理讲清。
原文为公有领域古籍;翻译、印象画与图文解读由 AI 辅助生成,鲲侯审校。