Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), in which the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is a partner, have finally found clear evidence that the supermassive black hole at the center of the Milky Way, Sagittarius A*(Sgr A*), is blowing a hot cosmic wind — something scientists have been hunting for over 50 years.

Astronomical theory says that when a black hole feeds on gas, it should also blow some material back out as winds or jets. Until now, the wind coming from our own Galaxy’s black hole had never been seen clearly. Using several years of highly detailed ALMA observations, astronomers mapped cold gas within just a few light‑years of Sgr A*. After carefully removing the black hole’s bright radio glow, they uncovered a giant, cone‑shaped hole in the cold gas, pointing straight at the black hole — the unmistakable imprint of a large, hot, active wind launched from Sgr A*.

Over five years of ALMA observations (made at a wavelength of 1.3 millimeters) astronomers mapped emission from carbon monoxide (CO) molecules, a classic tracer of cold molecular gas, within only about one parsec (or three light‑years) of Sgr A*. By carefully modeling and subtracting the black hole’s own rapidly varying radio emission, they were able to reveal extremely faint, intricate structures in the surrounding gas. Data from NASA’s Chandra X-Ray Observatory show hot gas filling the same region, confirming that this is a black hole–powered outflow, not something caused by nearby stars.

The map created from this ALMA data is about 100 times deeper and 80 times sharper than previous CO images of the region, making it the most sensitive, highest‑resolution map of cold gas within one parsec of Sgr A* ever obtained. This discovery relied not only on years of ALMA observations but also innovative data‑processing techniques to model and subtract Sgr A*’s rapidly variable emission, revealing fainter structures in the surrounding gas.

The team estimates this wind has been blowing for at least 20,000 years, but it’s relatively gentle compared to the dramatic jets seen in other galaxies. By revealing this long‑sought wind, ALMA (and Chandra) have helped solve a decades‑old mystery and given scientists their clearest view yet of how a supermassive black hole can both feed on and reshape its surroundings at the heart of our Milky Way Galaxy.

About ALMA

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science and Technology Council (NSTC) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.

About NRAO

The National Radio Astronomy Observatory (NRAO) is a facility of the U.S. National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.