2MASX J09431201+3155438, UGC 5190, MCG +05-23-029, PGC 27800, CGCG 152-058
NGC 2968 is a barred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,804±19km/s, which corresponds to a Hubble distance of 86.8±6.1Mly (26.61±1.88Mpc). However, five non-redshift measurements give a much closer mean distance of 45.69±13.40Mly (14.010±4.107Mpc). It was discovered by German-British astronomer William Herschel on 7 December 1785.
NGC 2968 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
SN 1970L (TypeIb/c, mag. 15.5) was discovered by Swiss astronomer Paul Wild on 31 October 1970. The supernova was found on the connecting bridge between NGC 2968 and NGC 2970, implying that the progenitor of SN 1970L was likely to have been accelerated by the tidal interaction of the two galaxies.
Compact galaxy group
NGC 2970 (center) with NGC 2970 (upper left) and NGC 2964 (lower right)
↑Barbon, R.; Ciatti, F.; Rosino, L. (1973). "Observations of five supernovae". Memorie della Societa Astronomica Italiana. 44: 65. Bibcode:1973MmSAI..44...65B.
↑"SN 1970L". Transient Name Server. IAU. Retrieved 24 December 2025.
↑Barton, Elizabeth; Geller, Margaret; Ramella, Massimo; Marzke, Ronald O.; Da Costa, L. Nicolaci (1996). "Compact Group selection from Redshift Surveys". The Astronomical Journal. 112: 871. arXiv:astro-ph/9608091. Bibcode:1996AJ....112..871B. doi:10.1086/118060.