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ALMA Delivers Record‑Size Image of Milky Way’s Central Molecular Zone

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ALMA Composite Reveals 650‑Light‑Year Gas Swath On 25 February 2026 the Atacama Large Millimeter/submillimeter Array in Chile released the largest stitched‑together image ever produced by the facility, mapping a cold‑gas region that spans more than 650 light‑years across the Galactic Center [1]. The observation focuses on the Milky Way’s Central Molecular Zone, a dense reservoir of star‑forming material previously unresolved at this scale [1]. The image was assembled from data collected by the full array of ALMA antennas, taking advantage of the desert’s exceptionally dry atmosphere [1].

Gas and Dust Encircle Sagittarius A* Black Hole – The new picture shows extensive clouds of gas and dust orbiting the galaxy’s central supermassive black hole, Sagittarius A*, highlighting the extreme physical conditions that dominate the region [1]. Researchers note that the zone is “a place of extremes, invisible to our eyes, but now revealed in extraordinary detail,” underscoring the unprecedented clarity of the millimeter‑wave view [1]. These structures provide a direct view of the material feeding and interacting with the black hole, a key component of Galactic dynamics [1].

Scientists Anticipate New Insights Into Galactic Evolution Survey leader Steve Longmore of Liverpool John Moores University states that analyzing star birth within this detailed map will improve understanding of how galaxies evolve over cosmic time [1]. European Southern Observatory astronomer Ashley Barnes emphasizes that the region’s extreme environment offers a natural laboratory for testing theories of star formation under high pressure and turbulence [1]. The data set is expected to feed multiple follow‑up studies, potentially reshaping models of the Milky Way’s past and future development [1].

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Timeline

Oct 2025 – Gemini South telescope on Cerro Pachón captures high‑resolution data of the Butterfly Nebula, providing the raw observations later processed into a detailed image [2].

Nov 26, 2025 – NSF’s NoirLab releases the processed Butterfly Nebula photograph, marking the International Gemini Observatory’s 25th anniversary and noting that Chilean schoolchildren chose the nebula as the target [2].

2025 – Astronomers identify the Butterfly Nebula as a planetary nebula 2,500‑3,800 light‑years away, powered by a central white dwarf whose expelled gas forms the characteristic butterfly‑shaped wings [2].

Feb 25, 2026 – ALMA in the Atacama Desert produces the largest composite image ever assembled, revealing a 650‑light‑year‑wide swath of cold molecular gas in the Milky Way’s Central Molecular Zone [1].

Feb 25, 2026 – The new ALMA image shows dense gas and dust clouds encircling the galaxy’s central supermassive black hole, delivering unprecedented detail of an extreme environment previously invisible to the eye [1].

Feb 25, 2026 – Survey leader Steve Longmore states the study “will clarify how star formation in the Central Molecular Zone drives galaxy evolution,” highlighting the image’s scientific significance [1].

Feb 25, 2026 – ESO researcher Ashley Barnes describes the region as “a place of extremes, invisible to our eyes, but now revealed in extraordinary detail,” underscoring the breakthrough in observational capability [1].

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