A galaxy cluster is a structure made up of hundreds to thousands of galaxies bound together by gravity, typically weighing from 10^14 to 10^15 solar masses.
Overview
Famous Galaxy Clusters
Observing Galaxy Clusters
What Is A Galaxy Cluster
Galaxy Cluster Classification
Galaxy Clusters And Cosmology
Components Of A Galaxy Cluster
Future Research On Galaxy Clusters
Formation And Evolution Of Galaxy Clusters
The Role Of Dark Matter In Galaxy Clusters
James Webb Space Telescope
Hubble Space Telescope
Dark Energy
Dark Matter
Universe
Gravity
Perseus
Matter
Magnet
Virgo
๐ A galaxy cluster is like a big neighborhood for hundreds to thousands of galaxies!
๐ Galaxy clusters can be super heavy, weighing about 1,000,000,000,000,000 times heavier than our Sun!
๐ Dark matter makes up about 80% of the mass in galaxy clusters and helps keep galaxies together.
๐ซ Galaxy clusters form when smaller groups of galaxies are pulled together by gravity.
๐ Clusters like the Virgo and Coma are famous examples that house many galaxies.
๐ญ Astronomers use special telescopes, like the Hubble Space Telescope, to observe galaxy clusters.
๐ก๏ธ The space between galaxies in clusters contains super-hot gas that glows brightly.
๐ค Galaxy clusters can grow by attracting and merging with other clusters, like galaxies making new friends.
๐ Scientists classify galaxy clusters as regular or irregular based on their shape and organization.
๐ Observing galaxy clusters helps researchers learn about the universe's history and its evolution.
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