SN 2004dj was the brightest supernova since SN 1987A at the time of its discovery.
This Type II-P supernova was discovered by Japanese astronomer Kōichi Itagaki on 31 July 2004. At the time of its discovery, its apparent brightness was 11.2 visual magnitude; the discovery occurred after the supernova had reached its peak magnitude. The supernova's progenitor is a star in a young, compact star cluster in the galaxy NGC 2403, in Camelopardalis. The cluster had been cataloged as the 96th object in a list of luminous stars and clusters by Allan Sandage in 1984; the progenitor is therefore commonly referred to as Sandage 96. This cluster is easily visible in a Kitt Peak National Observatory image and appears starlike.
References
External links supernovae.net image collection NASA Astronomy Picture of the Day: Cropped and rotated HST photograph (7 September 2004) Bright Supernova page on 2004dj


![SN 2004dj: A light curve for SN 2004dj, plotted from AAVSO data[2]](https://upload.wikimedia.org/wikipedia/commons/thumb/9/9c/SN2004djLightCurve.png/1280px-SN2004djLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
