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.

Mynd/Myndskeið:

ESO/Gravity Consortium/L. Calçada

Um myndina

Auðkenni:eso1835a
Tegund:Uppdráttur
Útgáfudagur:Okt 31, 2018, 10:00 CET
Tengdar fréttatilkynningar:eso1835
Stærð:2970 x 2972 px

Um fyrirbærið

Nafn:Sagittarius A*
Tegund:Milky Way : Galaxy : Component : Central Black Hole
Flokkur:Illustrations
Quasars and Black Holes

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