Simulation of Material Orbiting close to a Black Hole
ESO’s exquisitely sensitive GRAVITY instrument has added further evidence to the long-standing assumption that a supermassive black hole lurks in the centre of the Milky Way. New observations show clumps of gas swirling around at about 30% of the speed of light on a circular orbit just outside a four million solar mass black hole — the first time material has been observed orbiting close to the point of no return, and the most detailed observations yet of material orbiting this close to a black hole.
This visualization uses data from simulations of orbital motions of gas swirling around at about 30% of the speed of light on a circular orbit around the supermassive black hole Sagittarius A*.Oikeudet:
ESO/Gravity Consortium/L. Calçada
|Julkaisupäivä:||31. lokakuuta 2018 10:00|
|Frame rate:||30 fps|
|Kategoria:||Quasars and Black Holes|