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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.

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Evidence · 3
Timeline

No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.

Connections · 1
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

Read the assembled narrativeContinue in StudioOpen TwinTwin does not start a decision from this kind of object.ShareSaveSaved objects are part of the authenticated projection, which is declared and not yet built.

/atlas?object=OBJECT_SAGITTARIUS_A_STAR