
Nova remnant
Encyclopedia

Nova
A nova is a cataclysmic nuclear explosion in a star caused by the accretion of hydrogen on to the surface of a white dwarf star, which ignites and starts nuclear fusion in a runaway manner...
, or from the bubbles of gas blasted away in a recurrent nova. It has an expansion velocity of around 1000 km/s, and has a lifetime of a few centuries. Considering their short lifetimes, nova remnants usually do not exist anymore by the time their light reaches us. Nova remnants are much less massive than supernova
Supernova
A supernova is a stellar explosion that is more energetic than a nova. It is pronounced with the plural supernovae or supernovas. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months...
remnants or planetary nebulae.
External links
- T Pyxidis Nova Remnant (HubbleSite)
- Double-star systems cycle between big and small blasts (The Carnegie Observatories)
- Nova Remnant comparison table (UOttawa)
- Nova Remnant (UOttawa)