|Right Ascension||00 : 42 : 43.1 (h:m:s)
|Declination||+41 : 16 : 04 (deg:m:s)
|Visual Brightness||5.8 (mag, max)
|Spectral type||SN type I pec
Supernova 1885, also later named S Andromedae (for the second variable to be discovered in constellation Andromeda), was the first supernova discovered beyond our Milky Way galaxy, on August 20, 1885, by Ernst Hartwig (1851-1923) at Dorpat Observatory in Estonia. It reached mag 6 between August 17 and 20, and it was independently found by several observers. However, only Hartwig realized its significance. It faded to mag 16 in February 1890.
It is the only supernova to now to have been recorded in the Andromeda galaxy, M31.
The remnant of SN 1885 was discovered more than 100 years later by R.A. Fesen et.al. (1989) with the 4-m Mayall telesope of Kitt Peak National Observatory on CCD exposures taken on November 10, 1988, using narrow band interference filters, because of its absorption caused by iron atoms (Fe I). Hamilton and Fesen (2000) have used the Hubble Space Telescope to image absorption of this supernova remnant, and found its diameter to be 0.55 +/- 0.15 arc seconds in the light of Fe II. They calculated from these observations that this remnant contains between 0.1 and 1.0 solar masses of iron.
Last Modification: May 24, 2012