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The central stars of planetary nebulae are very hot.
Only once a star has exhausted all its nuclear fuel can it collapse to such a small size, and so planetary nebulae came to be understood as a final stage of stellar evolution.
Spectroscopic observations show that all planetary nebulae are expanding.
This led to the idea that planetary nebulae were caused by a star's outer layers being thrown into space at the end of its life.

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