| SN 2023ixf | |
| Epoch: | J2000 |
| Type: | Supernova |
| Host: | Pinwheel Galaxy |
| Constellation: | Ursa Major |
| Discovery: | 21 million years ago (detected 19 May 2023, 17:27 UTC by Koichi Itagaki) |
| Mag V: | 10.8 (on 22 May 2023) |
| Distance: | 21 million ly |
| Progenitor: | Supergiant (M=–4.66) |
SN 2023ixf is a type II-L[1] [2] (core collapse) supernova located in the Pinwheel Galaxy. It was first observed on 19 May 2023 by Kōichi Itagaki and immediately classified as a type II supernova.[3] Initial magnitude at discovery was 14.9. After discovery, the Zwicky Transient Facility project found a precovery image of the supernova at magnitude 15.87 two days before discovery.[4] The supernova was about 21 million light-years from Earth and is expected to have left behind either a neutron star or black hole, based on current stellar evolution models.
The supernova is located near a prominent HII region, NGC 5461, in an outer spiral arm of the bright galaxy.
By 22 May 2023, SN 2023ixf had brightened to about magnitude 11. It could be seen in telescopes as small as 114mm and remained visible with backyard telescopes for several months. The supernova started to fade around 10 June 2023.
The last supernova that close to Earth occurred 9 years previously: SN 2014J in Messier 82, roughly 12 million light-years from Earth.
| SN 2023ixf | Pinwheel Galaxy (M101) | 6.4Mpc | 10.8 | ||
| 3.7abbr=onNaNabbr=on | 10.1[5] | ||||
| Pinwheel Galaxy (M101) | 6.4abbr=onNaNabbr=on | Ia | 9.9[6] |
Before becoming a supernova, the progenitor star is believed to have been a supergiant with an absolute magnitude in the near-infrared (814nm) of MF814W = –4.66.