Tianji: Difference between revisions
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!Star Names or Orders( |
!Star Names or Orders(Qing) |
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!Ho PENG YOKE<ref>P.-Y. Ho, “Ancient And Mediaeval Observations of Comets and Novae in Chinese Sources,” ''Vistas in Astronomy'', 5(1962), 127-225.</ref> |
!Ho PENG YOKE<ref>P.-Y. Ho, “Ancient And Mediaeval Observations of Comets and Novae in Chinese Sources,” ''Vistas in Astronomy'', 5(1962), 127-225.</ref> |
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!Yi Shitong<ref>Yi Shitong伊世同. ''Zhongxi Duizhao Hengxing Tubiao''中西对照恒星图表1950. Beijing: Science Press.1981: 56.</ref> |
!Yi Shitong<ref>Yi Shitong伊世同. ''Zhongxi Duizhao Hengxing Tubiao''中西对照恒星图表1950. Beijing: Science Press.1981: 56.</ref> |
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Based on catalogue in 18th century |
Based on catalogue in 18th century |
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!Pan Nai<ref name=":0">Pan Nai潘鼐. ''Zhongguo Hengxing Guance shi''中国恒星观测史[M]. Shanghai: Xuelin Pree. 1989. p226.</ref> |
!Pan Nai<ref name=":0">Pan Nai潘鼐. ''Zhongguo Hengxing Guance shi''中国恒星观测史[M]. Shanghai: Xuelin Pree. 1989. p226.</ref> |
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based on Xinyixiangfayao Star Map |
based on Huangyou Star Catalogue and Xinyixiangfayao Star Map |
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!SUN X. & J. Kistemaker<ref>Sun Xiaochun. & Kistemaker J. ''The Chinese sky during the Han''. Leiden: Brill. 1997, Pp241-6.</ref> |
!SUN X. & J. Kistemaker<ref>Sun Xiaochun. & Kistemaker J. ''The Chinese sky during the Han''. Leiden: Brill. 1997, Pp241-6.</ref> |
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Han Dynasty |
Han Dynasty |
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!Boshun Yang<ref name=":1">B.-S. Yang杨伯顺, ''Zhongguo Chuantong Hengxing Guance Jingdu ji Xingguan Yanbian Yanjiu'' 中国传统恒星观测精度及星官演变研究 (A Research on the Accuracy of Chinese Traditional Star Observation and the Evolution of Constellations), PhD thesis, (Hefei: University of Science and Technology of China, 2023). 261.</ref> |
!Boshun Yang<ref name=":1">B.-S. Yang杨伯顺, ''Zhongguo Chuantong Hengxing Guance Jingdu ji Xingguan Yanbian Yanjiu'' 中国传统恒星观测精度及星官演变研究 (A Research on the Accuracy of Chinese Traditional Star Observation and the Evolution of Constellations), PhD thesis, (Hefei: University of Science and Technology of China, 2023). 261.</ref> |
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before Tang dynasty |
before Tang dynasty |
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!Boshun Yang<ref name=":1" /> |
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Yuan Dynaty (1363) |
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| 1st/Determinative |
| 1st/Determinative |
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| upsilon CrB |
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| xi CrB |
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| xi CrB |
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| xi CrB |
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| xi CrB |
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|zeta Her |
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| 2nd |
| 2nd |
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| xi |
| xi CrB |
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| zeta Her |
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| nu2 Her |
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| zeta Her |
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| nu1 Her |
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|53 Her |
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| 3rd |
| 3rd |
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| zeta Her |
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| epsilon Her |
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| zeta Her |
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| 53 Her |
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| zeta Her |
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|epsilon Her |
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|4th |
|4th |
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|53 Her |
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|d Her |
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|epsilon Her |
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| ⚫ | |||
|epsilon Her |
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|delta Aur |
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|epsilon Her |
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|alpha Cam |
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|u her |
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|5th |
|5th |
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| epsilon Her |
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| 61 Her |
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| d Her |
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| d Her |
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| d Her |
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|w Her |
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|6th |
|6th |
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|d Her |
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|u her |
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|w Her |
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| ⚫ | |||
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|u her |
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|u her |
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| ⚫ | |||
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|7th |
|7th |
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|c Her |
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|HIP 24479 |
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|Her 86178 |
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|11 Cam |
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|HIP |
|HIP 85382 |
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|theta Her |
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|12 Lyn |
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|theta Her |
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|7 Cam |
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|theta Her |
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|8th |
|8th |
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|u her |
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|? |
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|31 Cam |
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|theta Her |
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|HIP 24914 |
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|kappa Lyr |
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|15 Lyn |
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|kappa Lyr |
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|9 Aur |
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| ⚫ | |||
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|9th |
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|theta Her |
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|theta Her |
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|f Her |
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|mu Lyr |
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|kappa Lyr |
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Revision as of 10:51, 6 December 2025
Tiān Jì (Celestial Discipline, 天紀) consists of nine stars forming an east–west alignment that extends across the modern constellations Corona Borealis, Hercules, and Lyra. This asterism and the coordinate of its determinative star was first recorded in the Western Han Shishi xingjing (Master Shi’s Star Canon, 石氏星經).
Concordance, Etymology, History
Tianji is also called Jì xīng (Decipline Star). The term jì (紀) originally denoted “a thread of silk,” later acquiring the metaphorical meanings of “order,” “law,” or “discipline.” Hence, the Shishi zan (Commentary of Shi) explains: “The nine stars of Tiān Jì regulate litigation.” The ancients believed that by observing this asterism, one could divine whether the legal order of the empire remained upright and just.
Another interpretation, however, regarded the nine stars of Tianji as representing the Nine States (which are the major component of ancient China). According to this view, any unusual phenomenon observed in the asterism—such as brightening, dimming, or disappearance—portended terrestrial disasters such as earthquakes or mountain collapses.
Because most of its component stars are faint, the ancient astronomers considered any abnormal changes in their visibility—whether excessive brightness, darkness, or disappearance—as inauspicious omens.
Identification of stars
| Star Names or Orders(Qing) | Ho PENG YOKE[1] | Yi Shitong[2]
Based on catalogue in 18th century |
Pan Nai[3]
based on Huangyou Star Catalogue and Xinyixiangfayao Star Map |
SUN X. & J. Kistemaker[4]
Han Dynasty |
Boshun Yang[5]
before Tang dynasty |
Boshun Yang[5]
Yuan Dynaty (1363) |
|---|---|---|---|---|---|---|
| 1st/Determinative | upsilon CrB | xi CrB | xi CrB | xi CrB | xi CrB | zeta Her |
| 2nd | xi CrB | zeta Her | nu2 Her | zeta Her | nu1 Her | 53 Her |
| 3rd | zeta Her | epsilon Her | zeta Her | 53 Her | zeta Her | epsilon Her |
| 4th | 53 Her | d Her | epsilon Her | epsilon Her | epsilon Her | u her |
| 5th | epsilon Her | 61 Her | d Her | d Her | d Her | w Her |
| 6th | d Her | u her | w Her | u her | u her | HIP 85382 |
| 7th | c Her | Her 86178 | HIP 85382 | theta Her | theta Her | theta Her |
| 8th | u her | ? | theta Her | kappa Lyr | kappa Lyr | HIP 88836 |
| 9th | theta Her | theta Her | f Her | mu Lyr | kappa Lyr |
Maps (Gallery)
| historical map | modern identification | same in Stellarium 25.3 |
|---|---|---|
Star Name Discussion (IAU)
In 2025, the name of the historical constellation Bā Gǔ (八穀) was suggested to WGSN to be used for one of the stars in this constellation based on a review of Chinese cultural astronomy literature. Discussion focused on the bright star Delta Aurigae, which was the determinative star following multiple published versions of the asterism.
WGSN adopted the name "Bagu" for the bright star designated Delta Aurigae (HR 2077, HD 40035, HIP 28358) on 12 November 2025.
Bagu is a bright (V=3.72 mag) star at distance 43 parsecs. Since the middle of the 20th century, the star served as a Morgan-Keenan spectral standard for K0 giants. The star has a diameter about 12 times larger than that of our Sun. The star is a single-lined spectroscopic binary catalogued in SBC9, i.e. it has a faint companion on a period of 3.51 years (Griffin 2009). Specifically the name is applied to the primary Aa.
References
- ↑ P.-Y. Ho, “Ancient And Mediaeval Observations of Comets and Novae in Chinese Sources,” Vistas in Astronomy, 5(1962), 127-225.
- ↑ Yi Shitong伊世同. Zhongxi Duizhao Hengxing Tubiao中西对照恒星图表1950. Beijing: Science Press.1981: 56.
- ↑ Pan Nai潘鼐. Zhongguo Hengxing Guance shi中国恒星观测史[M]. Shanghai: Xuelin Pree. 1989. p226.
- ↑ Sun Xiaochun. & Kistemaker J. The Chinese sky during the Han. Leiden: Brill. 1997, Pp241-6.
- ↑ 5.0 5.1 B.-S. Yang杨伯顺, Zhongguo Chuantong Hengxing Guance Jingdu ji Xingguan Yanbian Yanjiu 中国传统恒星观测精度及星官演变研究 (A Research on the Accuracy of Chinese Traditional Star Observation and the Evolution of Constellations), PhD thesis, (Hefei: University of Science and Technology of China, 2023). 261.




