Pandora's Cluster

4 million lydiameter

Updated

4.00million ly
Visual creditMagellan and Hubble 2006 / NASA, ESA, and R. Dupke (Eureka Scientific, Inc.), et al. / Public domainSource: Wikimedia Commons

Details

Pandora's Cluster, also known as Abell 2744, is a giant galaxy cluster shaped by a violent and complicated merger of smaller clusters. Its galaxies, superheated gas, and dark matter have been pulled apart and redistributed in different ways, so astronomers can compare where the ordinary matter and the dark matter ended up.

Pandora's Cluster, Abell 2744, is the product of a complex merger involving several galaxy-cluster components. The galaxies, X-ray-emitting gas and mass reconstructed from gravitational lensing occupy different distributions because they responded differently during the collisions.

That separation lets astronomers compare ordinary matter with the dark-matter-dominated mass map. The cluster also acts as a gravitational lens, magnifying more distant galaxies behind it.

Key facts

Category
Galaxy clusters
Object class
Galaxy cluster
Scale fact
4 million lydiameter
Composition
Several hundred galaxies, hot intracluster gas, dark matter
Embed

Size neighbors

Objects near Pandora's Cluster on the scale

On the logarithmic size axis, Pandora's Cluster falls between Abell 1689 and Bullet Cluster. The band uses nearby Galaxy cluster records.

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

Sources

References for Pandora's 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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