`Guest Star' of AD 185
Identification of the `Guest Star' of AD185 as a comet rather than a supernova

Y.-N. Chin
Radioastronomisches Institut der Universität Bonn
Auf dem Hügel 71, D-53121 Bonn, Germany
and Y.-L. Huang
Institute of History, National Tsing Hua University
Hsinchu 30043, Taiwan

Paper published on29 September 1994 by Nature in vol 371, pp.398 - 399. If you want to have a look at the complete paper please click here (PostScript file of 1015542 bytes).
Abstract. Very few nearby suprenova have been bright enough to see with the naked eye. The only such case this century was Supernova 1987A. Matching historical records of such events with presently observable remnants allow accurate estimates to be made of the age and incidence rate of supernovae; ancient Chinese astronomical records are a particularly valuable resource for this purpose. In the Houhanshu of the Later Han dynasty is recorded the appearance of a `guest star' in AD 185. This is widely regarded as the oldest supernova recorded historically, and several candidate remnants have been suggested, in particular the object RCW86. Here we show that a reinterpretation of the relevant passage in the Houhanshu is inconsistent with the supernova interpretation, but suggests instead that the guest star was a comet. Our findings indicate that some of the keywords used by Chinese astronomers in historical records must be interpreted with caution.

Any suggestion or comments please e-mail to einmann@asiaa.sinica.edu.tw.

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