iPTF14hls

iPTF14hls

Supernova iPTF14hls before and after detection
Observation data
Epoch J2000      Equinox
Constellation Ursa Major
Right ascension 09h 20m 34.30s
Declination +50° 41′ 46.80″
Apparent magnitude (V) 17.716 (R)
Astrometry
Distance156,200,000 pc (509,000,000 lypc
Database references
SIMBADdata

iPTF14hls is an unusual supernova star that erupted continuously for about 1,000 days beginning in September 2014 before becoming a remnant nebula. It had previously erupted in 1954. None of the theories nor proposed hypotheses fully explain all the aspects of the object.