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Como Explorar o Explorador 3D do Efeito Yarkovsky

Abra o Explorador 3D do Efeito Yarkovsky, escolha um sentido de rotacao no seletor e avance ou reproduza o controle de anos decorridos enquanto o ponto quente de atraso termico de um asteroide irregular em rotacao empurra o anel orbital para dentro ou para fora.

  1. Abra https://freetoolonline.com/space-3d/yarkovsky-effect.html e aguarde o asteroide, o marcador do Sol e o anel orbital aparecerem.
  2. Use o seletor de rotacao para escolher Retrograda (Bennu, medida) ou Prograda (espelho didatico).
  3. Arraste o controle de anos decorridos (0-100) ou clique em "Play / Pause Years" para ver o anel orbital encolher (retrograda) ou crescer (prograda).
  4. Observe a seta de empuxo de recuo no ponto quente - vermelha quando o empuxo encolhe a orbita, verde quando a faz crescer.
  5. Leia o painel de fatos para a taxa com sinal da rotacao atual, a leitura de deriva acumulada e os numeros reais medidos de Bennu.
  6. Troque o sentido de rotacao e compare as duas animacoes do anel orbital lado a lado.

Principais numeros publicados

NumeroValor
Deriva do semieixo maior de Bennu-284,6 +/- 1,5 m/ano (Chesley et al. 2014, refinado pela JPL pos-OSIRIS-REx)
Deslocamento medido 1999-2012cerca de 160-185 km
Magnitude do empuxo"quase o peso de tres uvas" (NASA JPL)
Faixa de tamanho dominanteasteroides com cerca de 10 m a 10 km

A seguir: o guia de quando usar ou comparacao com alternativas. Abra o Explorador 3D do Efeito Yarkovsky.

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