Sagittarius A* - the black hole at the centre of the Milky Way
node · earth · Galactic centre, constellation Sagittarius as seen from Earth
The compact radio source at the dynamical centre of our own galaxy, about 8.3 kiloparsecs away, whose mass of roughly four million solar masses is known more securely than that of any other black hole because individual stars have been tracked around it for three decades. The Event Horizon Telescope published an image on 12 May 2022 showing a ring about 51.8 microarcseconds across, in close agreement with the size the stellar-orbit mass predicts - two entirely independent methods, one Newtonian celestial mechanics applied to stars, one general-relativistic light bending, converging on the same object. It was much harder to image than M87* despite being far closer, because its far smaller mass means the material orbits in minutes rather than days, so the source changes during the observation. Getting an image at all required averaging over many reconstructions and treating the variability explicitly. It is also extremely faint for its mass, accreting at a tiny fraction of the Eddington rate. Not a place on Earth.
Read in · 1
Evidence · 3
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
- A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 1
- M87* - the supermassive black hole in Messier 87comparable_to
Assembled narrative · 1
An assembled narrative is available for this object.
Observed changes · 0
No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.
Actions
/atlas?object=OBJECT_SAGITTARIUS_A_STAR