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.

Oikeudet:

ESO/Gravity Consortium/L. Calçada

Kuvasta

Tunnistus:eso1835a
Tyyppi:Kuvitus
Julkaisupäivä:31. lokakuuta 2018 10:00
Vastaavat julkaisut:eso1835
Koko:2970 x 2972 px

Kohteesta

Nimi:Sagittarius A*
Tyyppi:Milky Way : Galaxy : Component : Central Black Hole
Kategoria:Illustrations
Quasars and Black Holes

Kuvaformaatit

Suuri JPEG
2,5 MB
Kokoruudun JPEG
250,3 KB

Zoomattavissa


Taustakuvat

1024x768
190,2 KB
1280x1024
329,0 KB
1600x1200
510,9 KB
1920x1200
649,5 KB
2048x1536
876,7 KB