The Sun is crucial for life on Earth, but it won't last indefinitely; eventually, we'll need to seek a new home. The Sun's stability matters, yet it will deplete its nuclear fuel and turn into a white dwarf.
Larger stars expire more quickly, but the Sun's end will be comparatively tame. It has roughly 9 to 10 billion years remaining, over half of which has elapsed.
As it approaches its demise, the Sun will swell into a red giant, possibly engulfing Earth or altering its orbit to a warmer zone. Within 500 million to 1 billion years, Earth will become uninhabitable, necessitating a move.
The pace of evolution on Earth may shed light on the Fermi Paradox; stars with longer lifespans might harbor advanced civilizations.
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