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The event horizon

node

The one-way surface of a black hole: the boundary of the region from which no signal, however energetic, can reach a distant observer. It is a feature of spacetime and not an object - there is nothing there to touch, no wall, no density change, and no local experiment an infalling observer could perform to detect the moment of crossing. The horizon is defined globally, by where light rays end up in the infinite future, which means its position depends on the entire future history of what falls in; a horizon can grow outward in anticipation of matter that has not arrived yet. For a non-rotating hole it sits at the Schwarzschild radius; for a rotating one it lies between half that and the full value, shrinking as spin increases. Hawking showed in 1971 that under classical general relativity the total area of horizons never decreases, a result whose formal resemblance to the second law of thermodynamics turned out not to be a coincidence. Not a place on Earth.

A node is not a place. Drawing it on a map would assert something about the world that no stored fact supports.

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Evidence · 3
Timeline

No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.

Connections · 2
Assembled narrative · 1

Assembled from 31 blocks · 3 evidence · 29 related

  1. Story
  2. The one-way surface of a black hole: the boundary of the region from which no signal, however energetic, can reach a distant observer. It is a feature of spacetime and not an object - there is nothing there to touch, no wall, no density change, and no local experiment an infalling observer could perform to detect the moment of crossing. The horizon is defined globally, by where light rays end up in the infinite future, which means its position depends on the entire future history of what falls in; a horizon can grow outward in anticipation of matter that has not arrived yet. For a non-rotating hole it sits at the Schwarzschild radius; for a rotating one it lies between half that and the full value, shrinking as spin increases. Hawking showed in 1971 that under classical general relativity the total area of horizons never decreases, a result whose formal resemblance to the second law of thermodynamics turned out not to be a coincidence. Not a place on Earth.
  3. Knowledge
  4. Schwarzschild radius
  5. The event horizon
  6. The Kerr solution and black hole spin
  7. Connections
  8. The Kerr solution and black hole spin
  9. Schwarzschild radius
  10. Black hole entropy
  11. Schwarzschild solves the field equations for a point mass
  12. Oppenheimer and Snyder compute continued gravitational contraction
  13. Penrose proves that collapse to a singularity is generic
  14. The term "black hole" enters use
  15. GW150914 - two black holes merge and the signal reaches Earth
  16. The event horizon
  17. The no-hair result
  18. Innermost stable circular orbit
  19. Kerr finds the rotating solution
  20. A mechanism for extracting energy from a spinning black hole
  21. Karl Schwarzschild
  22. The event horizon
  23. The photon sphere and the shadow
  24. Time dilation near a horizon
  25. Tidal stretching near a black hole
  26. Einstein presents the field equations of general relativity
  27. Schwarzschild solves the field equations for a point mass
  28. Evidence
  29. The first exact solution of the Einstein field equations for the vacuum outside a spherical mass, containing the radius now named for its author. V55 VERIFICATION BASIS: the paper was NOT consulted in this session - WebFetch was refused by the network egress proxy for every host attempted and the WebSearch budget was exhausted before authoring began. Title, venue and page range are given from the author's recall of a canonical citation and must be checked.
  30. Establishes that geodesic incompleteness follows generically from the formation of a trapped surface, without an assumption of symmetry. V55 VERIFICATION BASIS: not consulted in session; no research tool was available. Volume and page are from recall of a canonical citation and must be checked.
  31. 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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