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 visualisation 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 black hole.

Autorska prava:

ESO/Gravity Consortium/L. Calçada

O slici

Id:eso1835a
Tip:Ilustracija
Datum objavljivanja:31. oktobar 2018. 10:00
Povezana saopštenja:eso1835
Veličina:2970 x 2972 px

O objektu

Naziv:Sagittarius A*
Tip:Milky Way : Galaxy : Component : Central Black Hole
Kategorija:Illustrations
Quasars and Black Holes

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