The Coma Berenices galaxy cluster is a dense grouping of thousands of galaxies visible in the constellation Coma Berenices, best viewed in the evening in April and May.
Located approximately 320 million light-years away, the cluster spans about 20 million light-years in space, housing galaxies of various shapes and sizes.
The Coma Berenices cluster contains as many as 10,000 galaxies, making it one of the most populated galaxy clusters known to scientists.
Elliptical galaxies are prominent in the cluster, with giant ellipticals like NGC 4889 and NGC 4874 being two to three times larger than the Milky Way.
Dark matter was discovered in the Coma Berenices galaxy cluster by Fritz Zwicky in the 1930s, indicating its significant mass contribution to the universe.
The cluster's center is located at approximately RA: 12h 59m, dec: +27° 59′ and is moving away from us at over 15 million mph (24 million kph).
Telescopes reveal a myriad of galaxies in the Coma Berenices cluster, with elliptical galaxies dominating the central region and spiral galaxies found farther out.
The region of the sky where the cluster is located is known as the Realm of the Galaxies, showcasing the vastness and complexity of this galactic grouping.
The Coma Berenices galaxy cluster played a significant role in the discovery of dark matter, a mysterious substance that affects the universe's evolution and fate.
Although not visible to the naked eye, the cluster's historical and scientific importance underscores its unique place in understanding the cosmos.