The first image of a black hole shadow is published
node
The Event Horizon Telescope Collaboration released an image of M87* in simultaneous press conferences and a series of papers in the Astrophysical Journal Letters: an asymmetric bright ring about 42 microarcseconds across surrounding a dark centre. The dark region is the shadow cast by strong light bending near the photon sphere, not the horizon itself, and it is about two and a half times larger in diameter. The measured diameter yielded a mass of roughly six and a half billion suns, agreeing with the higher of two competing pre-existing estimates. Four imaging teams had worked independently and blind before comparing results.
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Evidence · 2
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 5
- M87* - the supermassive black hole in Messier 87concerns
- The photon sphere and the shadowevidence_for
- Event Horizon Telescopeconcerns
- Accretion discconcerns
- Very long baseline interferometryconcerns
Assembled narrative · 1
Assembled from 51 blocks · 2 evidence · 32 related
- Story
- The Event Horizon Telescope Collaboration released an image of M87* in simultaneous press conferences and a series of papers in the Astrophysical Journal Letters: an asymmetric bright ring about 42 microarcseconds across surrounding a dark centre. The dark region is the shadow cast by strong light bending near the photon sphere, not the horizon itself, and it is about two and a half times larger in diameter. The measured diameter yielded a mass of roughly six and a half billion suns, agreeing with the higher of two competing pre-existing estimates. Four imaging teams had worked independently and blind before comparing results.
- Knowledge
- The photon sphere and the shadow
- Accretion disc
- M87* - the supermassive black hole in Messier 87
- Very long baseline interferometry
- Event Horizon Telescope
- The first image of a black hole shadow is published
- Connections
- The Event Horizon Telescope observes M87* and Sagittarius A*
- M87* - the supermassive black hole in Messier 87
- The photon sphere and the shadow
- Event Horizon Telescope
- Accretion disc
- Very long baseline interferometry
- Relativistic jet
- Sagittarius A* - the black hole at the centre of the Milky Way
- Heber Curtis records a curious straight ray in Messier 87
- A mechanism for extracting energy from a spinning black hole
- 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
- 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
- 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
- Innermost stable circular orbit
- Relativistic jet
- Cygnus X-1
- Cygnus X-1 is localised and weighed
- Bekenstein assigns entropy to a black hole
- The first image of a black hole shadow is published
- The M87* ring is imaged in polarised light
- A second epoch shows the ring persists and the bright spot moves
- Event Horizon Telescope
- The Event Horizon Telescope observes M87* and Sagittarius A*
- The first image of a black hole shadow is published
- Evidence
- Reports the first image of a black hole shadow, an asymmetric ring about 42 microarcseconds across, together with the array, observing campaign and imaging methodology. V55 VERIFICATION BASIS: not consulted in session; WebFetch to iopscience.iop.org and eventhorizontelescope.org was refused by the egress proxy and no search could be issued. Volume and article number are from recall of a canonical citation.
- Relates the measured ring diameter to the mass of M87*, giving approximately six and a half billion solar masses and testing the shadow prediction of general relativity. V55 VERIFICATION BASIS: not consulted in session; no research tool was available. Volume and article number are from recall; the quoted mass uncertainty is not reproduced in this pack.
Observed changes · 0
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