The black hole at the centre of our own galaxy is imaged
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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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Connections · 4
Assembled narrative · 1
Assembled from 42 blocks · 1 evidence · 26 related
- Story
- 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.
- Knowledge
- The photon sphere and the shadow
- Sagittarius A* - the black hole at the centre of the Milky Way
- S2 - the star that measured the Galactic centre
- Event Horizon Telescope
- The black hole at the centre of our own galaxy is imaged
- Connections
- Sagittarius A* - the black hole at the centre of the Milky Way
- Event Horizon Telescope
- The photon sphere and the shadow
- S2 - the star that measured the Galactic centre
- M87* - the supermassive black hole in Messier 87
- S2 - the star that measured the Galactic centre
- A star is tracked through a complete close approach to the Galactic centre
- The Event Horizon Telescope observes M87* and Sagittarius A*
- S2 passes pericentre and its light is measurably redshifted
- The orbit of S2 is shown to precess as general relativity predicts
- The Nobel Prize in Physics recognises black holes twice over
- The black hole at the centre of our own galaxy is imaged
- The Event Horizon Telescope observes M87* and Sagittarius A*
- Very long baseline interferometry
- Atacama Large Millimeter/submillimeter Array
- South Pole Telescope
- The Event Horizon Telescope observes M87* and Sagittarius A*
- The first image of a black hole shadow is published
- The M87* ring is imaged in polarised light
- The black hole at the centre of our own galaxy is imaged
- A second epoch shows the ring persists and the bright spot moves
- Schwarzschild radius
- The first image of a black hole shadow is published
- The black hole at the centre of our own galaxy is imaged
- A second epoch shows the ring persists and the bright spot moves
- Sagittarius A* - the black hole at the centre of the Milky Way
- A star is tracked through a complete close approach to the Galactic centre
- S2 passes pericentre and its light is measurably redshifted
- The orbit of S2 is shown to precess as general relativity predicts
- The Nobel Prize in Physics recognises black holes twice over
- The black hole at the centre of our own galaxy is imaged
- Evidence
- Reports an image of Sagittarius A* with a ring diameter of about 51.8 microarcseconds, consistent with the mass derived from stellar orbits, and describes the variability that made the imaging difficult. V55 VERIFICATION BASIS: not consulted in session; no research tool was available. Volume and article number are from recall and must be checked.
Observed changes · 0
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