Back اسان ۳۸۶ Persian SN 386 French SN 386 Japanese SN 386 Dutch SN 386 Portuguese G11.2-0.3 Russian SN 386 Swedish SN 386 Ukrainian
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| Event type | Supernova, supernova remnant  |
|---|---|
| Type II | |
| Date | April/May 386 |
| Constellation | Sagittarius |
| Right ascension | 18h 11.5m [1] |
| Declination | −19° 25′[1] |
| Distance | 14000-23000 LY |
| Remnant | Shell |
| Host | Milky Way |
| Other designations | SN 386 |
| Preceded by | SN 185 |
| Followed by | SN 393 |
 Related media on Commons | |
SN 386 is a probable transient astronomical event in the constellation Sagittarius, which appeared as a "guest star" that was reported by Chinese astronomers in 386 CE.[2]
- ^ a b Galactic SNRs: Detailed Listings
- ^ Clark, D. H.; Stephenson, F. R. (1976). "Which Historical New Stars were Supernovae?". Q. J. R. Astron. Soc. 17: 290. Bibcode:1976QJRAS..17..290C.
The position of the star AD 386 corresponds very well with that of the SNR G11.2–0.3, and this leads us to make the tentative suggestion that this source is the remnant of the star.