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The first image of a black hole shadow is published

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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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Connections · 5
Assembled narrative · 1

Assembled from 51 blocks · 2 evidence · 32 related

  1. Story
  2. 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.
  3. Knowledge
  4. The photon sphere and the shadow
  5. Accretion disc
  6. M87* - the supermassive black hole in Messier 87
  7. Very long baseline interferometry
  8. Event Horizon Telescope
  9. The first image of a black hole shadow is published
  10. Connections
  11. The Event Horizon Telescope observes M87* and Sagittarius A*
  12. M87* - the supermassive black hole in Messier 87
  13. The photon sphere and the shadow
  14. Event Horizon Telescope
  15. Accretion disc
  16. Very long baseline interferometry
  17. Relativistic jet
  18. Sagittarius A* - the black hole at the centre of the Milky Way
  19. Heber Curtis records a curious straight ray in Messier 87
  20. A mechanism for extracting energy from a spinning black hole
  21. The Event Horizon Telescope observes M87* and Sagittarius A*
  22. The first image of a black hole shadow is published
  23. The M87* ring is imaged in polarised light
  24. A second epoch shows the ring persists and the bright spot moves
  25. Schwarzschild radius
  26. The first image of a black hole shadow is published
  27. The black hole at the centre of our own galaxy is imaged
  28. A second epoch shows the ring persists and the bright spot moves
  29. The Event Horizon Telescope observes M87* and Sagittarius A*
  30. Very long baseline interferometry
  31. Atacama Large Millimeter/submillimeter Array
  32. South Pole Telescope
  33. The Event Horizon Telescope observes M87* and Sagittarius A*
  34. The first image of a black hole shadow is published
  35. The M87* ring is imaged in polarised light
  36. The black hole at the centre of our own galaxy is imaged
  37. A second epoch shows the ring persists and the bright spot moves
  38. Innermost stable circular orbit
  39. Relativistic jet
  40. Cygnus X-1
  41. Cygnus X-1 is localised and weighed
  42. Bekenstein assigns entropy to a black hole
  43. The first image of a black hole shadow is published
  44. The M87* ring is imaged in polarised light
  45. A second epoch shows the ring persists and the bright spot moves
  46. Event Horizon Telescope
  47. The Event Horizon Telescope observes M87* and Sagittarius A*
  48. The first image of a black hole shadow is published
  49. Evidence
  50. 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.
  51. 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.
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