JWST Identifies Cooling Gas in Phoenix Cluster 1z6a3r Unlocking Star Formation Process

JWST’s observations confirm missing cooling gas in the Phoenix Cluster, explaining its rapid star formation rate. 442fg

Written by Gadgets 360 Staff | Updated: 20 February 2025 18:00 IST

JWST Identifies Cooling Gas in Phoenix Cluster, Unlocking Star Formation Process

Photo Credit: Wikimedia Commons o1y2q

James Webb Space Telescope Reveals Phoenix Cluster's Cooling Mystery, Aiding Star Formation Research

Highlights

JWST detects cooling gas in Phoenix Cluster, aiding star formation
Phoenix Cluster holds the largest hot gas reservoir in the universe
Researchers confirm cooling gas in cluster cavities using MIRI

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Observations from the supermassive black hole at its core. Researchers have confirmed that the cluster contains the largest known reservoir of hot gas cooling at different rates.

JWST's Role in Identifying the Missing Cooling Gas 5o5743

According to a study published in Nature, data from JWST's Mid-Infrared Instrument (MIRI) has allowed researchers to locate gas cooling at 540,000 degrees Fahrenheit (300,000 degrees Celsius). This gas was found trapped in cavities within the cluster, an area previously unobservable.

Michael McDonald, an astrophysicist at the Massachusetts Institute of Technology (MIT) and principal investigator of the study, told Space.com that earlier studies failed to detect this gas because only the extreme temperature ends of the spectrum were measurable.

Webb Telescope Unveils Hidden Process Behind Star Formation in Phoenix Cluster

Supermassive Black Hole and Star Formation in Phoenix Cluster 2h66h

Despite a central black hole over 10 billion times the mass of the Sun, the Phoenix Cluster continues forming stars at an unprecedented rate. The discovery of trapped cooling gas helps explain this paradox.

The findings challenge previous assumptions about galaxy cluster cooling processes and suggest that similar techniques could be used to study other clusters. The researchers aim to apply these methods to further understand cooling mechanisms in space.

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