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White supergiants are luminous, A-class supergiants that have evolved off from the main-sequence age, when they were once O-class stars. They are expected to keep swelling in size but cooling in temperature, gradually turning yellow, then a deep red supergiant of over a terameter in diameter, before exploding into a catastrophic supernova.

See Also[]

Supergiant Stars
M · K · G · F · A · B · O
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