Sky science

Dark Nebula

Direct answer

Dark Nebula: A Dark Nebula is a dense interstellar cloud visible mainly because its dust blocks or reddens background light.

It appears as a silhouette against brighter stars or emission.

Astronomy & SkywatchingThe Great Almanac DictionaryUpdated 2026-09-26

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At a glance

Found in
Astronomy & Skywatching
Related
Emission Nebula, Reflection Nebula, Open Star Cluster, Globular Cluster
Observable sky · visual guide Dark Nebula

It appears as a silhouette against brighter stars or emission.

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The story behind Dark Nebula

Wide-field photography made many dust lanes conspicuous against the Milky Way.

A one-minute story

The Wandering Stars

How the moving planets were watched, named and found, and what a transit is.

Planet means wanderer.

Why Dark Nebula matters

Dark Nebula marks cold material where molecules and future stars can form.

Dark Nebula in practice: an example

The Horsehead Nebula appears dark against glowing hydrogen behind it.

Where readings of Dark Nebula go wrong

An apparently empty patch may contain abundant gas and dust rather than no stars.

Sources and editorial method

Research references used for this entry include:

Source
The Great Almanac Dictionary
Category
Astronomy & Skywatching
Last updated
2026-09-26

Look into a dark molecular cloud

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Emission NebulaIt produces its own spectral-line light. Reflection NebulaIt shines by reflected starlight rather than ionized-gas emission. Open Star ClusterIt is a sparse stellar family in a galactic disk. Globular ClusterIt is a compact ancient stellar population. AstronomyAstronomy is the science of celestial objects, space, and the physical universe. SkywatchingSkywatching is direct observation of the changing day and night sky.

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Common questions

What is a Dark Nebula?

A Dark Nebula is a dense interstellar cloud visible mainly because its dust blocks or reddens background light.

What do people get wrong about a Dark Nebula?

An apparently empty patch may contain abundant gas and dust rather than no stars.

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