The international collaboration of EHT astronomers proved this Thursday in image the existence of a black hole supermassive at the heart of our galaxy, Sagittarius A*, three years following the first photo of a black hole, located in a distant galaxy.
Evidence for scientists
The “silhouette” of the black hole silhouetted once morest a luminous disc of matter recalls that of the black hole of the distant galaxy M87, which is much larger than ours. Scientists see this as proof that the same mechanisms of physics are at work at the heart of two systems of very different sizes.
“I can show you the image of the Sgr A* black hole at the center of the galaxy,” EHT project manager Huib Jan Van Langevelde announced to applause at a press conference in Garching, Germany. Germany.
An extremely dense object
Technically, you can’t see a black hole, because the object is so dense and its gravitational force so powerful that not even light can escape from it. But we can observe the material that circulates around, before being swallowed.
“We have direct evidence that this object is a black hole,” explained Sara Issaoun of the Harvard Center for Astrophysics, describing “the cloud of gas (around the black hole) which emits radio waves and which we have observed “. Black holes are said to be stellar when they have the mass of a few suns, or supermassive when they have a mass of millions or even billions of suns.
Named Sagittarius A*
Sagittarius A* (Sgr A*), which owes its name to its detection in the direction of the constellation of Sagittarius, has a mass of approximately four million suns and is 27,000 light years from Earth. Its existence has been assumed since 1974, with the detection of an unusual radio source at the center of the galaxy.
The EHT, an international network of eight radio-astronomical observatories, had brought in 2019 the historic image of M87 *, a supermassive black hole of six billion solar masses in its galaxy, Messier 87, located at 55 million years. -light. With its four million solar mass, Sgr A* is a featherweight in the bestiary of supermassive black holes.
