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Sagittarius A* Star Orbit 3D Explorer vs Kepler Orbits 3D Explorer


Ver uma orbita real e medida leva um carregamento de pagina no Sagittarius A* Star Orbit 3D Explorer - 0 MB instalado, USD 0, sem conta. O Kepler Orbits 3D Explorer permite ajustar qualquer excentricidade de 0 a 0.97 numa elipse generica de Sol e planeta, mas nao renderiza um sistema real e publicado especifico.


Os numeros lado a lado

AspectoSagittarius A* Star Orbit 3D ExplorerKepler Orbits 3D Explorer
Tamanho de instalacao0 MB - roda no navegador0 MB - roda no navegador
Tempo para a primeira vistaSegundos - um carregamento de paginaSegundos - um carregamento de pagina
PrecoUSD 0USD 0
O que renderizaUma orbita real e publicada (S2 ao redor de Sagittarius A*, e ~0.88, 16.05 anos)Qualquer excentricidade 0-0.97 numa elipse generica de ensino Sol-e-planeta
Veja fatos Sagittarius A*: 0 MB de instalacao, carrega em segundos, USD 0, orbita real S2 e~0.88.
0 MB instalacao, segundos, USD 0, orbita S2 e~0.88.

Onde Sagittarius A* Star Orbit vence

Sagittarius A* Star Orbit vence quando a pergunta e "como os astronomos realmente mediram a massa de um buraco negro" - cada valor no seu painel e um numero publicado especifico de uma campanha de observacao real, nao um exemplo de ensino ajustavel.


Onde Kepler Orbits vence

Kepler Orbits vence quando a pergunta e sobre a forma geral das leis de Kepler - ajustar o controle de excentricidade de um quase-circulo a uma lasca cometaria em tempo real torna a propria geometria a licao, independente de qualquer sistema real.


Uma regra razoavel

Como regra razoavel, use Kepler Orbits primeiro para construir intuicao sobre o que a excentricidade faz a um caminho, depois use Sagittarius A* Star Orbit para ver essa mesma geometria aplicada a um sistema real e medido com uma medicao de massa em jogo. Para o proprio buraco negro renderizado artisticamente, use Black Hole 3D Explorer.

Veja quando usar Sagittarius A* Star Orbit 3D Explorer para adequacao de sessao.

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