Supernova

Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months. During this short interval a supernova can radiate as much energy as the Sun is expected to emit over its entire life span

1. Multiwavelength X-ray, infrared, and optical compilation image of Kepler’s supernova remnant, SN 1604

2. The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova

3. SN 1994D, a type Ia supernova in the NGC 4526 galaxy (bright spot on the lower left)

4. Multiwavelength composite image of the remnant of Tycho’s supernova, SN 1572.

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