Bullet Cluster

6.3 million lyobserved field width

Updated

6.30million ly
Visual creditMagellan and Hubble 2006 / NASA / CXC / M. Weiss / Public domainSource: Wikimedia Commons

Details

The Bullet Cluster is a pair of colliding galaxy clusters whose components have been torn apart by impact. Its galaxies and most of its mass passed through relatively cleanly, while the hot ordinary gas lagged behind, making the system one of astronomy’s clearest pieces of evidence that most matter in galaxy clusters is dark matter.

In the Bullet Cluster, two galaxy clusters have passed through one another. Their hot gas collided, slowed and remained near the center, while the galaxies crossed with much less resistance.

Gravitational-lensing maps place most of the mass near the galaxies rather than the X-ray-bright gas, which contains most of the ordinary matter. That spatial separation is strong evidence for a collisionless dark-matter component, although the displayed 6.3-million-light-year size is the width of the observed field rather than a physical cluster boundary.

Key facts

Category
Galaxy clusters
Object class
Colliding galaxy clusters
Scale fact
6.3 million lyobserved field width
Composition
~40 galaxies, hot intracluster gas, dark matter
Embed

Size neighbors

Objects near Bullet Cluster on the scale

On the logarithmic size axis, Bullet Cluster falls between Pandora's Cluster and Perseus Cluster. The band uses nearby Galaxy clusters records.

Shared physical scale
15.3million ly
Abell 16892.4 million ly
Pandora's Cluster4 million ly
Bullet Cluster6.3 million ly
Perseus Cluster11.6 million ly
Virgo Cluster15 million ly
Coma Cluster20 million ly

Sources

References for Bullet Cluster

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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