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SN 2002bj was the explosion of a star in the galaxy NGC 1821, located in the constellation Lepus.[2] The explosion was discovered by Jack Newton in scans of images produced by Tim Puckett. (It was independently discovered by the Lick/Tenagra Observatory as part of their combined supernova search program.) Initially it had an apparent magnitude of about 14.7[3] and was categorized as a Type IIn supernova.[4] However, in 2008 Dovi Poznanski discovered that the spectrum more closely resembled a Type Ia supernova. Further, the energy output was much lower than a typical supernova and the luminosity dropped at a dramatic pace.[5]

SN 2002bj

Event type	Supernova, variable star
SN.IIn
Constellation	Lepus
Right ascension	05h 11m 46.41s[1]
Declination	−15° 08′ 10.8″[1]
Epoch	J2000
Other designations	SN 2002bj, AAVSO 0507-15
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A team consisting of Poznanski, Joshua Bloom, Alex Filippenko and others concluded that it was a new category of exploding star. This system is believed to consist of a binary pair of white dwarf stars, with helium being transferred from one dwarf to the other. The accreted helium exploded in a thermonuclear reaction on the surface of the more massive white dwarf, resulting in the observed outburst.[5] In this sense, it was akin to a nova explosion, although the magnitude of the explosion was a thousand times greater.[2] In 2007 Lars Bildsten et al. had predicted this category of explosion would occur in AM Canum Venaticorum star binary systems.[6]

NGC 1821 is an irregular galaxy categorized as type IB(s)m. It is apparent magnitude 14.5 and has a redshift of 0.012029. This galaxy is located about 48 megaparsecs from the Earth.[7]

References

External links

• Light curves and spectra on the Open Supernova Catalog

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