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Bright and Dark: DECam’s New Shot of Coma Cluster

Bright and Dark: DECam’s New Shot of Coma Cluster

August 15, 2024
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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Bright and Dark: DECam’s New Shot of Coma Cluster

by nasaspacenews
August 15, 2024
in Galaxies, News, Others
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Bright and Dark: DECam’s New Shot of Coma Cluster

Coma Cluster galaxies. Source: CTIO/NOIRLab/DOE/NSF/AURA Image Processing: D. de Martin & M. Zamani (NSF NOIRLab)

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In 1937, Swiss astronomer Fritz Zwicky made a groundbreaking discovery within the Coma Cluster that would forever change the field of astrophysics. He noticed that the galaxies in this colossal cluster were moving far too fast for the visible mass to keep them gravitationally bound. This puzzling observation led Zwicky to propose the existence of an unseen force: “dark matter,” a mysterious substance that doesn’t emit or reflect light but exerts gravitational influence on visible objects.

Fast forward to today, and Zwicky’s once-radical theory is now a cornerstone of modern cosmology. Rubin’s observations of the Andromeda Galaxy provided further evidence of missing mass, confirming that dark matter is not only present in galaxy clusters but also across the entire universe. Thanks to advancements in technology, such as the powerful Dark Energy Camera (DECam), we now have a stunning new image of the Coma Cluster, offering not just a visual spectacle, but a deeper connection to the cosmic enigma that Zwicky first uncovered.

The recent DECam image of the Coma Cluster showcases the cluster’s immense size and complexity. The Coma Cluster is not made up of individual stars but entire galaxies, held together by gravity. However, as Zwicky discovered, the visible matter within the cluster is only a small fraction of what keeps it intact. Dark matter, though invisible, exerts enough gravitational pull to keep these galaxies bound together despite their rapid movement.

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The DECam itself is an extraordinary instrument. Originally built to carry out the Dark Energy Survey, this 570-megapixel camera was designed to study another great cosmic mystery. Dark energy, unlike dark matter, is the force believed to be driving the accelerated expansion of the universe. The camera, mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory, enables astronomers to probe deep into space, capturing detailed images of far-off galaxies and clusters like Coma.

As we look to the future, projects like the upcoming Legacy Survey of Space and Time (LSST) at the Vera C. Rubin Observatory promise to provide even more data on dark matter and dark energy. With the aid of advanced instruments like DECam and LSST, astronomers are closer than ever to unraveling the full story of dark matter—an invisible force that governs so much of the universe yet remains one of its greatest mysteries. The Coma Cluster, once a puzzle for astronomers, continues to be a key to unlocking these cosmic secrets.

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This Hubble image shows Omega Centauri, the Milky Way's largest globular clusters. Globular clusters contain some of the oldest stars in the Universe, and new research determines their absolute age. Image Credit: ESA/Hubble & NASA, M. Häberle (MPIA)

Astronomers Just Unlocked the Birth Dates of the Milky Way’s Oldest Stars

May 12, 2025
Image NASA’s Solar Dynamics Observatory captured this image of the Sun on May 7, 2024

There’s a Violent Solar Storm That Could Have Been Worse—Here’s the Scary Truth

May 11, 2025
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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This Hubble image shows Omega Centauri, the Milky Way's largest globular clusters. Globular clusters contain some of the oldest stars in the Universe, and new research determines their absolute age. Image Credit: ESA/Hubble & NASA, M. Häberle (MPIA)

Astronomers Just Unlocked the Birth Dates of the Milky Way’s Oldest Stars

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