Quote:
Originally Posted by Milky Way Resident
Are the Sirius double system and the Alpha Centauri triple one likely to produce at least a Type I supernova?
Sirius already has a white dwarf, whereas the Alpha binaries are of similar mass to the sun. What would happen to Proxima Centauri then? Red dwarfs are expected to last for trillions of years, but could a supernova in the Alpha Centauri system destroy Proxima?
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No.
First, it is very unlikely for the Alpha Centauri system to produce a supernova. None of the three stars is big enough to undergo a Type II supernova. Alpha Centauri A, being larger than Alpha Centauri B, will progress to white dwarf-dom first. A Type Ia supernova would then be theoretically possible, but A & B are currently far too distant for matter accretion to occur. A gravitational perturbation (from a passing system) would be required to nudge the two closer together. Possible - but very unlikely.
Second, Proxima Centauri (or, Alpha Centauri C) would not be harmed beyond perhaps losing a little stellar atmosphere. A supernova isn't a blast in the conventional sense that we understand one on Earth. Really, the term 'explosion' is what misleads us; it
is an explosion, but not as we conventional understand one to be. C would be bombarded by neutrinos and electromagnetic radiation, but it wouldn't be
impacted per se in any real physical way beyond its orbit increasing somewhat due to mass-loss by A going supernova.
Note:
Long before even the remote possibility of a supernova in the Alpha Centauri system could be realized, two things will have occurred: 1) the Sun will have long since rendered the Earth uninhabitable (this is expected to occur in less than a billion years, due to the gradual increase of the Sun's luminosity), and 2) Alpha Centauri will be somewhere else (compared to the Sun and the Earth) in the Milky Way, due to the galaxy's differential rotation.