The James Webb Space Telescope (JWST) was used to investigate the extreme cooling of gas in the Phoenix cluster, located around 5.8 billion light-years from Earth.
At the heart of the Phoenix cluster is a supermassive black hole 10 billion times as massive as the sun, yet stars continue to form at an incredible rate.
The JWST investigation aims to resolve the mystery of how star formation persists despite the presence of a supermassive black hole that should be hindering it.
Researchers liken the gas cooling in the Phoenix cluster to a ski slope, where not all the gas cools to low temperatures, analogous to skiers not making it down the mountain.
Using JWST's Mid-Infrared Instrument (MIRI), researchers located the 'missing skiers' or cooling gas contributing to star formation within cavities in the Phoenix Cluster.
The team found gas at around 540,000 degrees Fahrenheit located within cavities in the Phoenix Cluster, essential for star formation.
MIRI's sensitivity and ability to detect ionized neon and oxygen atoms in the Phoenix Cluster proved crucial in this investigation.
This research sheds light on the unique characteristics of the Phoenix Cluster and sets the stage for studying other galaxy clusters using similar techniques.
The team's findings were published on Feb. 5 in the journal Nature, offering valuable insights into the cooling mechanisms of gas in the Phoenix Cluster.