Linked from

The 46 pages that link to Supernova, each with the reason it gives.

• Stellar nucleosynthesisRelated: Explosions eject newly synthesized elements into the surrounding interstellar medium.

• Interstellar dustRelated: Some supernova ejecta form dust, while their shocks can also destroy existing grains.

• Stellar feedbackRelated: Supernovae inject energy, momentum, and newly synthesized elements into the interstellar medium.

• Gravitational binding energyRelated: The energy budget must overcome the binding of the star's outer layers and remnant.

• Chinese astronomyRelated: Historical Chinese observations include transient guest stars now identified as supernovae.

• Small Magellanic CloudRelated: Supernovae enrich its interstellar gas and drive energetic flows.

• Galactic windRelated: Overlapping supernovae can heat interstellar gas and drive it out of a galaxy.

• StarRelated: Some massive stars end in supernovae that disperse newly formed elements.

• Carina NebulaRelated: Past explosions may have contributed to the complex's energetic and turbulent environment.

• AntaresRelated: Antares is expected to end its life in a supernova, though not on a predictable human timescale.

• Circumstellar mediumRelated: Its ejecta collide with material lost by the star before the explosion.

• Eagle NebulaRelated: A disputed interpretation of X-ray evidence proposed that a past supernova shock contributed to pillar destruction.

• Pulsar planetRelated: The explosion that formed a pulsar would likely destroy any planets that existed around its progenitor.

• Arp 220Related: Rapid star formation in Arp 220 produces frequent supernovae that heat and stir its compact gas.

• Messier 81Related: The supernova SN 1993J in M81 became a major target for studying stellar explosions.

• Stellar astronomyRelated: Supernovae expose late-stage stellar processes and distribute newly formed elements.

• Local BubbleRelated: Supernovae are the leading explanation for the energy that excavated the cavity.

• PSR B1937+21Related: A supernova produced the neutron star that became PSR B1937+21.

• Super star clusterRelated: Supernovae from cluster members enrich and reshape the surrounding interstellar medium.

• Computational astrophysicsRelated: Simulations investigate explosion mechanisms that are difficult to observe from within.

• Intergalactic dustRelated: Supernovae produce dust and drive some grains out of galaxies.

• Sculptor GalaxyRelated: Supernovae help heat and accelerate the gas flowing from NGC 253's core.

• Zeta OphiuchiRelated: A supernova in its former binary system likely released the star from its orbit.