Credit: Credit: NASA, ESA, C. McCully and S. Jha (Rutgers Univ.), R. Foley
(University of Illinois), and Z. Levay (STScI)
Acknowledgment: Hubble Heritage Team (STScI/AURA), and A. Riess (JHU/STScI)
SUPERNOVA 2012Z IN SPIRAL GALAXY NGC 1309.
The inset panel is a pair of Hubble Space Telescope images of the spiral galaxy
NGC 1309 that were taken before and after the appearance of Supernova 2012Z,
in the outskirts of the galaxy. The white X-shaped feature at the top of the
image of the galaxy marks the location of the supernova.
The inset panel from 2013 shows the supernova; archival Hubble data from 2005
and 2006 show the progenitor system for the supernova, thought to be a binary
system containing a helium star transferring material to a white dwarf that
exploded.
The stellar blast is a member of a unique class of supernova called Type Iax.
These supernovae are less energetic, and hence fainter, on average, than their
well-known cousins, Type Ia supernovae, which also originate from exploding
white dwarfs in binary systems.