Sep 11, 2026

Webb Saw Water Survive Near the Milky Way's Black Hole

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There are places in the cosmos where we expect to find almost everything except chemical delicacy. The centre of the Milky Way is one of them. Even so, on 11 August 2026, ESA/Webb published a result that pushes against intuition: the James Webb Space Telescope found clear signs of water and oxygen-rich dust around the evolved star IRS 3, located only 0.55 light-years from Sagittarius A*, the supermassive black hole at the heart of our galaxy.

The discovery, explained by ESA/Webb and presented in an Astronomy & Astrophysics paper, does not say there are oceans near the black hole. It says something subtler and maybe more important: molecules and dust grains can form and persist in an environment dominated by intense radiation, stellar winds, and extreme gravity.

IRS 3 field observed by James Webb with NIRCam and MIRI data near Sagittarius A*
Webb combined NIRCam and MIRI data to observe the field containing IRS 3 near the galactic centre. Image: ESA/Webb, NASA & CSA, F. Peißker, J. Lu, F. Yusef-Zadeh, N. B. Sabha, C. Chan

What people are saying

The fast version of the news can sound almost miraculous: Webb found water next to a black hole. That line grabs attention, but it can also mislead. IRS 3 is not falling into Sagittarius A*, and the detected water is not a hidden lake at the centre of the galaxy. The star is in the asymptotic giant branch phase, a late stage of stellar life in which huge, cool objects shed material into space through powerful winds.

The useful myth, then, is imagining the galactic centre as a shredder that prevents any complex chemistry. The radiation is harsh, yes. The region is turbulent, yes. But the new Webb spectrum shows that the story is not only destruction. Evolved stars can keep making dust and molecules even in a cosmic neighbourhood that seemed too hostile.

Close-up image of the star IRS 3 captured by Webb
IRS 3 is one of the brightest mid-infrared sources in the galactic centre and has an unusually large dusty envelope. Image: ESA/Webb, NASA & CSA, F. Peißker, J. Lu, F. Yusef-Zadeh, N. B. Sabha, C. Chan

What the data says

The key is MIRI, Webb's mid-infrared instrument. According to the technical abstract, the team obtained the first continuous mid-infrared spectrum of IRS 3 in 2025 as part of the MICONIC programme. After correcting for dust extinction between us and the galactic centre, strong silicate signatures appeared: a broad band near 9.7 microns and another absorption feature around 18.5 microns. That pattern reclassifies IRS 3 as an oxygen-rich star.

Between 6 and 6.25 microns came the most surprising detail: signals consistent with water in the star envelope. The team also modelled the dust as a layered structure, with temperatures falling from about 1200 Kelvin close to the star to around 100 Kelvin in the outer regions. The estimated extent is roughly 10,000 astronomical units, a huge scale for material shed by a single star.

IRS 3 field seen by James Webb MIRI instrument
MIRI sees the galactic centre at wavelengths where dust, silicates, and infrared emission tell a different story from visible light. Image: ESA/Webb, NASA & CSA, F. Peißker, F. Yusef-Zadeh, N. B. Sabha, C. Chan

Why this changes the picture of the galactic centre

For decades, the centre of the Milky Way has been treated as a laboratory of extremes: compact stars, ionized clouds, magnetic fields, shocks, and the central black hole. The IRS 3 result adds a quieter piece. If evolved stars can return dust to the interstellar medium in this region, then the matter cycle that feeds future stars and planets may continue even where it once seemed interrupted.

The paper estimates that IRS 3 has about six solar masses and an age near 72 million years. The modelled mass-loss rate, assuming a 15 km/s wind, is approximately 6 x 10^-5 solar masses per year. In plain terms: the star is intensely enriching its surroundings, and Webb was able to read the composition of that material with a precision that previous observations did not have.

The verdict

The discovery matters now because it turns a popular image into something more complex. A supermassive black hole does not automatically erase every chemical process around it. There can be destruction, but also recycling. There can be extreme radiation, but also new dust. There can be a violent neighbourhood and, still, water held in the envelope of a dying star.

Webb did not find life at the centre of the galaxy, or a habitable refuge beside Sagittarius A*. It found a clue about cosmic resilience. And that clue is enough to change the question: not only "what survives near a black hole?", but "how much material essential for future stars and planets keeps forming where we thought almost nothing could endure?".

NIRCam star field of IRS 3 in the Milky Way centre
The NIRCam view highlights the stellar density and dust clouds that make the galactic centre difficult to interpret. Image: ESA/Webb, NASA & CSA, F. Peißker, J. Lu

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