description G292.0+1.8 Overview
G292.0+1.8 is a young, oxygen-rich supernova remnant in the constellation Centaurus. It contains rapidly moving stellar ejecta and a central pulsar surrounded by a pulsar wind nebula, produced by particles released by the neutron star. Oxygen-rich remnants are uncommon in the Milky Way, and G292.0+1.8 is commonly listed with Cassiopeia A and Puppis A among the three confirmed examples.
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How good is G292.0+1.8?
G292.0+1.8 scores 6.07/10 (Fair) on Lunoo, making it rated in the Nebula category.
What are the best alternatives to G292.0+1.8?
See our alternatives page for G292.0+1.8 for a ranked list with scores. Top alternatives include: N132D (LMC), MSH 15-52 (RCW 89), RCW 86 (SN 185).
How does G292.0+1.8 compare to N132D (LMC)?
See our detailed comparison of G292.0+1.8 vs N132D (LMC) with scores, features, and an AI-powered verdict.
Is G292.0+1.8 worth it in 2026?
With a score of 6.07/10, G292.0+1.8 is a solid option in Nebula. See all Nebula ranked.
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