Skip to main content
Log in

The identification of comets in Chinese historical records

  • Research Paper
  • Published:
Science China Physics, Mechanics and Astronomy Aims and scope Submit manuscript

Abstract

The historical records of astronomical phenomena may play a significant role in comet identification. Getting an accurate result is based on many factors, of which the calculation of orbital elements is the most important. This paper presents a “Cross Reference” method in which the perturbation of Jupiter is the only considered factor used to attempt an efficient way of comet identification with ancient Chinese historical records. In this method, the records before and after the calculated result from orbital determination within the error range are compared with the historical records to find the correlated perihelion time, and then, with five other orbital elements at the perihelion time, the ephemeris is calculated. If the calculated ephemeris matches the historical records, it is concluded that the comet determined by orbital calculation is the same as the one recorded in history. With this method, three comets with four historical records have already been found.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. Lu X W. Identification of cometary records in ancient China. Prog Astron, 2000, 18: 38–45

    ADS  Google Scholar 

  2. Hasegawa I. Orbits of ancient and medieval comets. Publ Astron Soc Jpn, 1979, 31: 257–270

    ADS  Google Scholar 

  3. Hasegawa I, Nakano S. Periodic comets found in historical records. Publ Astron Soc Jpn, 1995, 47: 699–710

    ADS  Google Scholar 

  4. Marsden B G. The next return of the comet of the Perseid meteors. Astron J, 1973, 78: 654–662

    Article  ADS  Google Scholar 

  5. Yao K, Yeomans D K, Weissman P. The past and future motion of Comet P/Swift-Tuttle. Mon Not R Astron Soc, 1994, 266: 305–316

    ADS  Google Scholar 

  6. Anderson J D, Esposito P B, Martin W, et al. Experimental test of general relativity using time-delay data from Mariner 6 and Mariner 7. Astrophys J, 1975, 200: 221–233

    Article  ADS  Google Scholar 

  7. Zhou J L. Celestial Mechanics. Nanjing: Nanjing University, 2005. 43–67

    Google Scholar 

  8. Hasegawa I, Nakano S. Orbit of periodic comet 153P/Ikeya-Zhang. Mon Not R Astron Soc, 2003, 345: 883–888

    Article  ADS  Google Scholar 

  9. Carusi A, Kresák Ľ, Kresáková M, et al. Observations of periodic comet d’Arrest in 1678 and implications for its evolutionary history. Astron Astrophys, 1991, 252: 377–384

    ADS  Google Scholar 

  10. Yeomans D K, Kiang T. The long-term motion of comet Halley. Mon Not R Astron Soc, 1981, 197: 633–646

    ADS  Google Scholar 

  11. Kresák Ľ, Kresáková M. Secular brightness decrease of periodic comets. Icarus, 1990, 86: 82–92

    Article  ADS  Google Scholar 

  12. Chin Y N, Huang Y L. Identification of the guest star of AD 185 as a comet rather than a supernova. Nature, 1994, 371: 398–399

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Gang Zhao.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Zhang, L., Zhao, G. The identification of comets in Chinese historical records. Sci. China Phys. Mech. Astron. 54, 150–155 (2011). https://doi.org/10.1007/s11433-010-4135-6

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11433-010-4135-6

Keywords

Navigation