Webb reveals metal-rich gas around Milky Way's central black hole

Researchers using the James Webb Space Telescope have discovered that gas orbiting the Milky Way's central black hole, Sagittarius A*, is rich in metals. This composition suggests the gas and nearby stars may have formed simultaneously.
Why it matters
Understanding the chemical makeup of material around black holes provides insights into galactic evolution and the distribution of heavy elements in the universe.
edited by Lisa Lock , reviewed by Robert Egan
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Add to Preferred Sources A swirling vortex of hot gas glows with infrared light, marking the approximate location of Sagittarius A. Credit: NASA, ESA, SSC, CXC, STScI The gas orbiting Sagittarius A (Sgr A*), the supermassive black hole at the center of the Milky Way galaxy, is rich in metals, researchers at McGill University's Trottier Space Institute have found. The metal enrichment probably resulted from stars that exploded and released material into the black hole's surroundings over time, they said.
The team also learned this gas is similar in composition to many of the stars in the black hole's orbit, suggesting the gas and stars may have formed together.
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