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Sh2-225 - Nebula
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Sh2-225

description Sh2-225 Overview

Sh2-225 is an emission nebula and H II region in the constellation Auriga. It lies in the Milky Way's Perseus Arm and is catalogued in the Sharpless list of H II regions. The region is associated with ionized hydrogen and an embedded infrared source, making it a subject of observations of massive-star formation; one proposed ionizing star is the O-type star LSV+4046. Because it is faint and compact in optical images, it is primarily of interest to astronomers and astrophotographers.

help Sh2-225 FAQ

How good is Sh2-225?
Sh2-225 scores 6.25/10 (Fair) on Lunoo, making it rated in the Nebula category. Obscure Sharpless object with limited imagery, faint appearance, and weak community recognition.
What are the best alternatives to Sh2-225?
See our alternatives page for Sh2-225 for a ranked list with scores. Top alternatives include: Sh2-91, Pickering's Triangle (NGC 6979), Simeis 147.
How does Sh2-225 compare to Sh2-91?
See our detailed comparison of Sh2-225 vs Sh2-91 with scores, features, and an AI-powered verdict.
Is Sh2-225 worth it in 2026?
With a score of 6.25/10, Sh2-225 is a solid option in Nebula. See all Nebula ranked.

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