Reflection nebula (NGC 1999), a real image
Image: NASA/ESA and the Hubble Heritage Team (STScI).

Types of Nebulae

Reflection Nebula

Example: NGC 1999

A cloud of dust that does not glow by itself but reflects the light of a nearby star, often looking blue.

Key facts

How it shines
Dust reflects light from a nearby star
Typical colour
Blue
Example shown
NGC 1999
Lit by
The young star V380 Orionis
Example’s distance
About 1,500 light-years

About the Reflection Nebula

How to recognise it

Reflection nebulae shine only because their dust reflects light from nearby stars. They often look blue, for a similar reason to the blue sky: blue light is scattered more easily.

The example: NGC 1999

NGC 1999, in the constellation Orion, is lit by a newborn star, V380 Orionis, near its centre. The dark keyhole shape was once thought to be a dense cloud blocking light, but observations by ESA’s Herschel space observatory showed it is an empty region of space. What made it is still unknown.

Sources

Facts checked: 29 October 2026