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NASA’s Chandra Observatory Helps Identify Hidden Treble Clef Galaxy Cluster

A peculiar formation of radio waves resembling a musical treble clef, hidden behind the crowded and dusty plane of the Milky Way, has been traced to a powerful supermassive black hole outburst followed by a violent galaxy cluster collision, according to findings published in the journal Astronomy & Astrophysics.

Unlocking the Treble Clef Radio Phoenix

Catalogued as VLSS J0318.9+5755, the looping structure sits in a region of the sky that astronomers have historically struggled to study, often referred to as the Zone of Avoidance. Because stars, gas, and dust in our galaxy block much of the view from Earth, researchers had to rely on advanced telescopes capable of seeing through this obscuring material to uncover the origin of the phenomenon.

Quick Look: NASA's Chandra Breaks Down 'Treble Clef's' Galaxy Cluster Collision

Two-Stage Cosmic Evolution

Led by Andrea Botteon of Italy’s National Institute for Astrophysics (INAF), a team of researchers determined that the Treble Clef developed across two primary stages. In the first phase, an active phase of the supermassive black hole at the center of the galaxy cluster ejected clouds of charged particles and magnetic fields outward at speeds approaching that of light. This activity produced bright radio emissions that eventually faded over time as the particles lost energy.

In the second stage, a massive collision between two galaxy clusters compressed and reenergized the old cloud of particles, causing it to light up again in radio light. Astronomers refer to this type of revived remnant as a “radio phoenix” because it rises from the fading ashes of an earlier outburst. Shock waves from the crash, similar to sonic booms produced by supersonic jets, may have also helped restore its brightness, while churning gas motions during the merger twisted the plasma into its distinctive filamentary shape.

Tour: NASA's Chandra Breaks Down 'Treble Clef's' Galaxy Cluster Collision

Multiple Telescopes Confirm Hot Gas Surrounds Treble Clef

The discovery required combining instruments operating across different wavelengths. Initial surveys spotted the object using LOFAR (Low Frequency Array), a European network of low-frequency radio antennas, with follow-up observations conducted using India’s Giant Metrewave Radio Telescope and the United Kingdom Infrared Telescope.

To characterize the surrounding environment, scientists turned to NASA’s Chandra X-ray Observatory and Germany’s eROSITA space telescope. These instruments detected widespread, multi-million-degree hot gas filling the cluster, confirming that the Treble Clef sits inside a massive galaxy cluster located about 1.6 billion light-years away. The data allowed researchers to pin down the cluster’s temperature, mass, and distance for the first time, revealing that the cluster weighs approximately 600 trillion times as much as our sun.

Astronomers spot something positively enormous behind the mi craw
Photo: Mashable SEA

Analysis of the hot gas shape—by removing a roughly oval symmetrical pattern from the X-ray images—showed stronger emissions on the left and right sides of the cluster’s center, indicating the direct collision occurred along a left-to-right axis. Researchers believe this crash took place a few hundred million years ago and that the two clusters are now moving away from each other.

Timeline of Discovery and Future Outlooks

The Treble Clef first surfaced in radio surveys years ago. Early speculation mistook it for a pulsar—a fast-spinning dead star—while a 2004 study linked it to a possible galaxy cluster without being able to resolve its shape. After fading from scientific literature, it appeared again in a 2022 list of potential “X-shaped” radio sources before the new LOFAR survey data revealed its twisting structure clearly.

While the black hole outburst and merger interpretation represents the team’s best analysis of the data, questions remain regarding the dynamics of cosmic rays and the faint radio halo detected exclusively by the Indian telescope at the cluster’s center. Researchers suggest the Treble Clef will serve as a prime target for sharper, very low-frequency follow-up observations using the upgraded LOFAR2.0 network.