A second epoch shows the ring persists and the bright spot moves
node
Analysis of the 2018 observing campaign produced a second image of M87*, published in 2024. The ring diameter was consistent with the 2017 result, as the geometry requires, since the shadow size is fixed by mass and distance. The position of maximum brightness around the ring had shifted, which the accretion flow permits and the geometry does not constrain. The pair of epochs is the cleanest available demonstration that the dark centre is a stable structural feature rather than an imaging artefact of one week of data.
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Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 4
- M87* - the supermassive black hole in Messier 87assesses
- Event Horizon Telescopeconcerns
- The photon sphere and the shadowconcerns
- Accretion discconcerns
Assembled narrative · 1
Assembled from 44 blocks · 1 evidence · 32 related
- Story
- Analysis of the 2018 observing campaign produced a second image of M87*, published in 2024. The ring diameter was consistent with the 2017 result, as the geometry requires, since the shadow size is fixed by mass and distance. The position of maximum brightness around the ring had shifted, which the accretion flow permits and the geometry does not constrain. The pair of epochs is the cleanest available demonstration that the dark centre is a stable structural feature rather than an imaging artefact of one week of data.
- Knowledge
- The photon sphere and the shadow
- Accretion disc
- M87* - the supermassive black hole in Messier 87
- Event Horizon Telescope
- A second epoch shows the ring persists and the bright spot moves
- Connections
- M87* - the supermassive black hole in Messier 87
- Event Horizon Telescope
- The photon sphere and the shadow
- Accretion disc
- 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
- 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
- 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
- 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.
Observed changes · 0
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