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Quando usar Tidal Disruption Event 3D Explorer

Use this explorer when you want to see how a supermassive black hole shreds a star - and skip it when you want the black hole itself or a moon torn apart by a planet.

  • Classroom demos of spaghettification and the tidal radius
  • Connecting the flare decline to the t^-5/3 fallback rate
  • Explaining why very massive black holes swallow stars whole

This is an educational visualization with illustrative sizes and a compressed timeline.


Evento de disrupcao de mare: numeros principais

Numeros principais do evento de disrupcao de mare em um painel: Tidal Disruption Event 3D Explorer lista a formula do raio de mare, cerca de metade da estrela acreta, declinio do flare t^-5/3 e engolir inteiro acima de ~10^8 massas solares.

Compare os numeros principais do evento de disrupcao de mare: o raio de mare, a massa acretada, o declinio do brilho e o limite de massa para engolir a estrela inteira.
Disrupcao de mare: raio de mare, massa acretada, declinio do brilho e limite de massa.
QuantidadeValor
Raio de marer_t = R_estrela x (M_BN / M_estrela)^(1/3)
Massa ligada que e acretadacerca de metade da estrela
Declinio do brilhot^-5/3
Massa limite para engolir a estrela inteiraacima de ~10^8 massas solares

Walk the controls in the step-by-step guide, or compare options in vs alternatives. Open the Tidal Disruption Event 3D Explorer.

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