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James Webb Detects Water in Dust Envelope of Dying Star Near Milky Way’s Center

WHY IT MATTERS

The finding shows that water can persist in the dust envelopes of evolved stars near the Galactic Center, offering fresh insight into the region’s chemical processes and the lifecycle of interstellar material.

What happened

On September 11, 2026, NASA’s James Webb Space Telescope captured a sharp image of IRS 3, a late‑stage star located in the dense starfield surrounding Sagittarius A*. Webb’s mid‑infrared observations revealed a clear signature of oxygen‑rich silicate dust in the star’s surrounding envelope and, for the first time, detected water vapor within that same dust cloud. The discovery confirms that water can survive in the harsh, high‑energy environment near the Milky Way’s supermassive black hole. It also provides a new laboratory for studying the chemistry of dust and gas in the Galactic Center, where conditions differ markedly from the quieter regions of the galaxy.

PRIMARY SOURCES

Dust and Water in Sagittarius A*

NASA · HQ Web Team · NASA media usage guidelines; third-party material excluded

CORRECTIONS & UPDATES

  1. Revision 1 · Initial ingestion · Sep 10, 2026, 4:45 PM
  2. Revision 2 · Source update detected · Sep 10, 2026, 4:45 PM
By THELAST.NEWS Editorial System · AI-assistedRevision 2Authoritative primary source