M87* and Sgr A* side-by-side in polarised light
Seen here in polarised light, this side-by-side image of the supermassive black holes M87* and Sagittarius A* indicates to scientists that these beasts have similar magnetic field structures. This is significant because it suggests that the physical processes that govern how a black hole feeds and launches a jet may be universal features amongst supermassive black holes.
The scale shows the apparent size on the sky of these images, in units of micro-arcseconds. A finger held at arm's length measures 1 degree on the sky; a micro-arcsecond is 3.6 billion times smaller than that. In context, the images of these black holes have an apparent size similar to that of a donut on the surface of the Moon.
Kredit:EHT Collaboration
O snímku
Id: | eso2406b |
Typ: | Koláž |
Datum zveřejnění: | 27. března 2024 14:00 |
Související články: | eso2406 |
Velikost: | 9600 x 5400 px |
O objektu
Jméno: | M87*, Sagittarius A* |
Typ: | Milky Way : Galaxy : Component : Central Black Hole Local Universe : Galaxy : Component : Central Black Hole |
Kategorie: | Quasars and Black Holes |
Image Formats
Barvy & filtry
Pásmo | Vlnová délka | Dalekohled |
---|---|---|
Milimetrový | 1.3 mm | Event Horizon Telescope |