NGC 6302 Hubble: Butterfly Emerges from Stellar Demise in Planetary Nebula NGC 6302

The central star itself cannot be seen, because it is hidden within a doughnut-shaped ring of dust, which appears as a dark band pinching the nebula in the center. The thick dust belt constricts the star's outflow, creating the classic "bipolar" or hourglass shape displayed by some planetary nebulae.

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