. In it, Geoffrey C Bower, the project scientist for the EHTC, described how Sagittarius A* was identified nearly 50 years ago as the nearest supermassive black hole candidate and ranks among theSagittarius A* “is the ultimate laboratory for black hole astrophysics”, Bower said. “These results are the culmination of a multi-year effort by the EHTC and a decades-long journey by the astronomy community to approach the event horizon through high-resolution imaging.
Although one cannot see the black hole itself, glowing gas around it shows a tell-tale signature: a dark central region, called a “shadow”, surrounded by a bright ring-like structure. “The new view captures light bent by the powerful gravity of the black hole, which is four million times more massive than our sun.”
Professor Roger Deane, the director of the Wits Centre for Astrophysics and extraordinary professor at the University of Pretoria, explained that Sgr A* is a 1 000 times faster black hole than M87*.
Truly extraordinary
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