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Recordeddatespace

The black hole at the centre of our own galaxy is imaged

The Event Horizon Telescope published an image of Sagittarius A* showing a ring about 51.8 microarcseconds across, from the same April 2017 campaign that produced the M87* result three years earlier. The delay was caused by the source itself: with a mass roughly fifteen hundred times smaller than M87*, its material orbits in minutes, so the structure changed during the observation and standard imaging methods smeared it. The recovered ring size matches the prediction from the mass measured by watching stars orbit - two independent methods agreeing on one object.

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Recorded on Sagittarius A* - the black hole at the centre of the Milky Way

  1. A star is tracked through a complete close approach to the Galactic centre
  2. The Event Horizon Telescope observes M87* and Sagittarius A*
  3. S2 passes pericentre and its light is measurably redshifted
  4. The first image of a black hole shadow is published
  5. The orbit of S2 is shown to precess as general relativity predicts
  6. The Nobel Prize in Physics recognises black holes twice over
  7. The M87* ring is imaged in polarised light
  8. The black hole at the centre of our own galaxy is imaged
  9. A second epoch shows the ring persists and the bright spot moves

Related

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