Eagle Nebula

70 lymaximum extent

Updated

70.0ly
Visual creditLa Silla Observatory 2009 / ESO / CC BY 4.0Source: Wikimedia Commons

Details

The Eagle Nebula is a young star-forming region in the Milky Way best known for the Pillars of Creation, towering columns of cold gas and dust sculpted by intense radiation from nearby massive stars. Beyond the famous pillars, it is a broad active nebula whose embedded cluster is steadily reshaping the surrounding cloud.

The Eagle Nebula is an emission nebula and star-forming molecular cloud containing the young cluster NGC 6611. Ultraviolet radiation and winds from its massive stars ionize the exposed gas and erode denser material around the cluster.

The Pillars of Creation are columns of comparatively cold gas and dust surviving inside that radiation field. Embedded young stars exist in and around the pillars, but the same radiation that reveals their environment is also dispersing the material from which additional stars could form.

Key facts

Category
Nebulae
Object class
Emission nebula
Host
Milky Way
Scale fact
70 lymaximum extent
Composition
Ionized hydrogen, molecular gas, dust, embedded star cluster
Temperature
~10,000 K ionized gas
Embed

Size neighbors

Objects near Eagle Nebula on the scale

On the logarithmic size axis, Eagle Nebula falls between Orion Nebula and Omega Centauri. The band uses nearby Emission nebula records.

Shared physical scale
53.5ly

Sources

References for Eagle Nebula

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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