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

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Tunnistus:eso1835b
Julkaisupäivä:31. lokakuuta 2018 10:00
Vastaavat julkaisut:eso1835
Kesto:15 s
Frame rate:30 fps

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