The light cone is a boundary beyond which nothing, not even light, can travel. Events on opposite sides remain disconnected. Yet spacetime itself is subject to quantum jitter: gravitational waves — quanta of quantum fields — ripple ceaselessly within it. This trembling acts like a desert heat haze, blurring the sharp edge of the light cone. Over millennia, the uncertainty builds up to entire meters.
Near a black hole, the haze thickens. Stephen Hawking and Jacob Bekenstein discovered that holes possess entropy — a measure of hidden complexity — and thus warm their surroundings. This robs the event horizon of its crispness: it is smeared by quantum uncertainty, and the near-hole space exists in a mix of geometries. If spacetime had Planck-scale temperature (10³² degrees), the haze would become so dense that light cones would lose all definition almost instantly — within 10⁻⁴³ seconds.
At room temperature, blurring the light cone by a meter would take 10,000 years; at Planck temperature, just 10⁻⁴³ seconds.