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Unveiling the Milky Way's Turbulent Core in Unprecedented Detail

Published on June 23, 2026, 7:59 p.m.
Unveiling the Milky Way's Turbulent Core in Unprecedented Detail

Topic: Space

Astronomers have created a stunning new image of the Milky Way's center using ALMA. The image shows intricate gas filaments and will help scientists understand star formation near the supermassive black hole.

A team of astronomers has produced an extraordinary image of the Milky Way's central region, revealing an intricate network of cosmic gas filaments in unprecedented detail. This massive map was created using the Atacama Large Millimeter/submillimeter Array (ALMA) and is the largest ALMA dataset ever assembled.

The image shows a region known as the Central Molecular Zone (CMZ), which stretches over 650 light-years across. It contains dense clouds of gas and dust that surround the supermassive black hole at the center of the Milky Way.

The new dataset reveals structures throughout the CMZ at many scales, from massive gas formations spanning dozens of light-years to small clouds surrounding individual stars. The survey responsible for this work is called ACES, which focuses specifically on cold molecular gas, the material that fuels star formation.

By analyzing the signals from this gas, researchers uncovered a surprisingly complex chemical environment. They detected dozens of molecules, including relatively simple ones such as silicon monoxide and more complex organic compounds like methanol, acetone or ethanol.

The CMZ hosts some of the most massive stars known in our galaxy, many of which live fast and die young, ending their lives in powerful supernova explosions, and even hypernovae. Through the ACES survey, researchers hope to learn how such violent environments influence the birth of stars and whether current theories of star formation remain valid under these extreme conditions.

Building the Largest ALMA Mosaic To gather this enormous dataset, astronomers used ALMA, a powerful observatory operated by ESO and its partners in Chile's Atacama Desert. This marks the first time such a large portion of the galactic center has been surveyed with ALMA, resulting in the observatory's largest image so far.

The final mosaic was created by combining many individual observations, much like assembling pieces of a puzzle. On the sky, the completed image spans a length equivalent to three full Moons placed side by side.

Why It Matters

This discovery can help us better understand how stars form and evolve in extreme environments, which is crucial for understanding the history and evolution of our galaxy. It also provides insights into the early Universe, where stars were forming in chaotic, extreme environments.

Key Facts

  • Astronomers have created a stunning new image of the Milky Way's central region using ALMA.
  • The image shows an intricate network of cosmic gas filaments and will help scientists understand star formation near the supermassive black hole.
  • The Central Molecular Zone (CMZ) stretches over 650 light-years across and contains dense clouds of gas and dust.
  • Researchers detected dozens of molecules, including relatively simple ones such as silicon monoxide and more complex organic compounds like methanol, acetone or ethanol.
  • The CMZ hosts some of the most massive stars known in our galaxy, many of which live fast and die young.

Key Terms

Supermassive black hole
A very large black hole at the center of a galaxy that has an enormous gravitational pull.

Implications

This discovery can help us better understand how stars form and evolve in extreme environments, which is crucial for understanding the history and evolution of our galaxy. It also provides insights into the early Universe, where stars were forming in chaotic, extreme environments.


Source: https://www.sciencedaily.com/releases/2026/03/260305182705.htm

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