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Quando Usar Redshift and Doppler Shift 3D Explorer - Melhores Sessoes e Limites

Last reviewed: 2026-07-14

O Redshift and Doppler Shift 3D Explorer e ideal para demonstracoes em sala de aula do diagrama de onda-Doppler, pausas rapidas de curiosidade sobre por que uma linha espectral se move, e para entender a lei de Hubble. E uma geometria educacional - nao um pipeline de espectroscopia - entao alguns tipos de sessao precisam de outra ferramenta.

Uma demonstracao de cinco minutos em sala de aula

Abra o Redshift and Doppler Shift 3D Explorer, pressione Aproximando e depois Afastando, e veja o marcador se mover pela barra espectral enquanto os pulsos de anel comprimem e se espalham.

Numeros em um unico painel

Mantenha a tabela de fatos visivel enquanto le z = v/c, o comprimento de onda de repouso do hidrogenio-alfa em 656.28 nm, e o exemplo da lei de Hubble a 100 Mpc.

Sessoes que nao se encaixam

Estas sessoes nao se encaixam no Redshift and Doppler Shift 3D Explorer: qualquer momento em que voce precise de estrutura galactica, mecanica orbital ou um passo a passo da escada de distancias. Use Milky Way Map 3D Explorer, Kepler Orbits 3D Explorer ou Parallax Distance 3D Explorer. Tambem precisa de WebGL no navegador.

← Back to Space 3D

Last updated: Jul 14, 2026

Reviewed by the Free Tool Online editorial team · Tested in the current versions of Chrome, Firefox, Safari, and Edge before publishing. No account is needed to use any tool. Report a bug - we triage within 72 hours. · Last refreshed April 2026.

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