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NGC 595 - Nebula
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NGC 595

description NGC 595 Overview

NGC 595 is a giant H II region in the Triangulum Galaxy, also called Messier 33, where ultraviolet radiation from young, massive stars ionizes surrounding hydrogen gas. Heinrich Louis d'Arrest discovered it in 1864. It is one of the largest star-forming nebulae in the Local Group and is studied by astronomers investigating massive stars, ionized gas, and stellar evolution outside the Milky Way.

help NGC 595 FAQ

What kind of object is NGC 595?

NGC 595 is a giant H II region, meaning a cloud of ionized hydrogen around young, massive stars. It lies in the Triangulum Galaxy, also called Messier 33.

Where is NGC 595 located?

It is located in the Triangulum Galaxy, or M33. M33 is one of the Local Group's nearby spiral galaxies.

Who discovered NGC 595?

Heinrich Louis d'Arrest discovered NGC 595 in 1864. The object was later recognized as a major star-forming nebula in M33.

Why is NGC 595 important to astronomers?

It is one of the largest star-forming nebulae in the Local Group. Ultraviolet light from young massive stars ionizes the surrounding hydrogen gas.

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