Novae

Nova means "new star", but they are actually "newly visible" stars caused by brightening of an existing star by 5 to 15 magnitudes. This can be brightening by hundreds of millions of times. The brightening may occur within a few days or weeks, but usually fades again within months. There are some recurring novae, but most are one-time events. One model of novae suggests that they occur in binary systems where one is a white dwarf and the other is on its way to becoming a red giant . The red giant can lose mass which would trigger hydrogen fusion as it falls on the white dwarf. This would blow the gas off and the process could repeat itself. A notable nova example is Nova Cygni 1975.

Index

Reference
Pasachoff
Ch. 7
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Nova Cygni 1975

The brightest Nova in recent years was Nova Cygni 1975 which became visible in Cygnus in August. It reached a magnitude of 1.8 after a rise in magnitude of about 15 in two days time. This is a million-fold increase in luminosity!
Index

Reference
Pasachoff
Ch. 7
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