ALMA puts a black hole on the scale
Illustration of a shock wave (bright "blob" in the upper jet) following a spiral path (in yellow) as it moves away from the black hole BL Lacertae. The blob plows through a section of the jet where the magnetic field (light blue curved lines) is wound up in a coil. This caused a brightening seen in visible, X-ray, and Gamma-ray light; later, the shock passed through the stationary X-shaped compression in the jet and brightened a second time.

ALMA puts a black hole on the scale

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How do you weigh a black hole?

For a person, it’s easy. You just step upon a scale and read off your weight. But no scale is large enough to carry a black hole! Even if it were, it would be gobbled up by the black hole’s incredible gravitational pull in no time.

Nevertheless, astronomers have now precisely determined the mass of a black hole in a distant galaxy. Not with a scale, but by measuring the rotational velocity of a disk of cold gas around the black hole, using ALMA.

The principle is well-known in astronomy. Take our own sun, for example. You can’t put it on a scale, but still, astronomers know how much it weighs. They only need to measure the orbital velocities of the planets. Mercury, the nearest planet, orbits the sun at some 48 kilometers per second. The Earth, though, only travels at 30 kilometers per second. And distant Neptune slowly crawls around at just some 5.5 kilometers per second.

If you know both a planet’s orbital velocity and its distance to the sun, it’s very straightforward to calculate the mass of the sun. The same is true for gas orbiting a black hole. Close to the black hole, where gravity is strong, the gas will move faster than far away from the black hole, where gravity is weaker.

ALMA was trained at a huge elliptical galaxy in the southern sky. From earlier measurements, it was already known that the galaxy harbors a massive black hole in its very core. Thanks to its sharp vision, ALMA could discern a rotating disk of cold gas surrounding the black hole. And by measuring the millimeter radiation of carbon monoxide molecules in the gas, the astronomers could determine the rotational velocity at various distances from the black hole.

From the observations, the astronomers calculated that the black hole in the galaxy’s core must weigh in at a stunning 2.25 billion times the mass of our own sun. It’s the highest black hole mass ever determined by ALMA.

About one out of every ten elliptical galaxies has a rotating disk of gas in its very center. Therefore, the astronomers hope that they will be able to weigh many more black holes, in other galaxies, using the same clever technique.


The large elliptical galaxy studied by ALMA is known as NGC 3258. It is at least 100 million light-years away from the Earth, in the southern constellation Antlia, the Air Pump. The galaxy was discovered in 1834 by astronomer John Herschel, who studied the southern sky from South Africa. Like all elliptical galaxies, NGC 3258 has a supermassive black hole in its core. The black hole is surrounded by a rotating disk of cold molecular gas. The new ALMA measurements revealed that the outer rim of this disk, some 500 light-years away from the black hole, moves around at about one million kilometers per hour. However, much closer in, at a distance of just 65 light-years from the black hole, the gas whirls around at well over three million kilometers per hour. From these measurements, it follows that the black hole’s mass must be some 2.25 billion times the mass of the sun.


The ALMA observations of NGC 3258 were carried out by a team of astronomers led by Benjamin Boizelle of the Texas A&M University in the United States. Benjamin worked together with his American colleagues Aaron Barth, Jonelle Walsh, David Buote, Andrew Baker and Jeremy Darling, and with Luis Ho from Peking University in China. The team has published their results in a paper in The Astrophysical Journal.

Check this in ALMA site