description Simeis 147 Overview
Simeis 147 is a vast filamentary nebula located in the Taurus region of the Milky Way. It represents the expanding remains of a supernova explosion that occurred approximately 9,000 years ago. The remnant’s immense size – spanning roughly three degrees – makes it particularly notable for astronomers studying stellar death and the evolution of galaxies. PSR J0538+2817, a pulsar, is embedded within this nebula, offering insights into extreme magnetic fields generated by collapsed stars.
This object is primarily studied by researchers investigating supernova remnants and their associated phenomena.
insights Why this score
Simeis 147 ranks #90 of 577 in the Nebula ranking, behind NGC 604, ahead of Ghost of Jupiter Nebula.
Simeis 147 has iconic filamentary structure, strong scientific interest, and high astrophotography prestige.
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