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.
Crédit:EHT Collaboration
À propos de l'image
Identification: | eso2406b |
Type: | Collage |
Date de publication: | 27 mars 2024 14:00 |
Communiqués de presse en rapport: | eso2406 |
Taille: | 9600 x 5400 px |
À propos de l'objet
Nom: | M87*, Sagittarius A* |
Type: | Milky Way : Galaxy : Component : Central Black Hole Local Universe : Galaxy : Component : Central Black Hole |
Catégorie: | Quasars and Black Holes |
Image Formats
Couleurs & filtres
Domaine | Longueur d'onde | Télescope |
---|---|---|
Millimétrique | 1.3 mm | Event Horizon Telescope |