Objects · Milky Way scale

Nebula

A cloud of interstellar gas and dust. Nebulae are the birthplaces of new stars and the glowing remnants of stars that have died. Five main types: emission, reflection, dark, planetary, and supernova remnant.

Notable example

The Orion Nebula (M42), just 1,344 light-years away, is a stellar nursery containing over 1,000 young stars in various stages of formation — visible to the naked eye.

Source: HubbleSite Nebulae

Nebulae — cradles and graves of stars

The word nebula (Latin: cloud) was once applied to any fuzzy, extended sky object — including what we now know to be distant galaxies. Today it refers specifically to interstellar clouds of gas (mostly hydrogen and helium) and dust within a galaxy. They are the raw material from which stars form and the enriched material returned when stars die.

The full story of how nebulae connect to the stellar life cycle is told in our what is a nebula guide and the stellar life cycle guide. Nebulae are the origin of solar systems — including ours: see how the Solar System formed.

Quick facts

Orion Nebula size
~24 ly across
Main component
Hydrogen gas
Visible types
5 main types

Frequently asked questions

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