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Como Explorar o Venus Runaway Greenhouse Explorer 3D

Abra o Venus Runaway Greenhouse Explorer 3D, arraste o controle deslizante de CO2 ou pressione Reset, e veja por que uma camada espessa de CO2 mantém Vênus mais quente que Mercúrio, mesmo Vênus orbitando quase duas vezes mais longe do Sol.

  1. Abra https://freetoolonline.com/space-3d/venus-runaway-greenhouse.html e aguarde Vênus renderizar.
  2. Arraste o controle de CO2 para longe de 96% e observe a camada de neblina em torno de Vênus ficar mais fina e mudar de cor.
  3. Pressione "Reset" para voltar o controle à composição real medida de Vênus (96,5% de CO2) e leia a temperatura de superfície real de 464 C / 737 K no painel de dados.
  4. Ative a comparação com Mercúrio para ver uma esfera de Mercúrio em escala ao lado de Vênus, e leia por que Mercúrio - quase duas vezes mais próximo do Sol - ainda é mais frio em média.
  5. Ative as barras de comparação de pressão para ver a pressão de superfície de Vênus (92 bar) ao lado da Terra (1 bar) e de Mercúrio (quase zero).
  6. Leia o painel de dados para a tabela completa de todos os dados publicados usados nesta página.

Principais dados publicados

FigureValue
Venus surface temperatureabout 464 C (737 K), day and night
Venus surface pressureabout 92 bar
Venus atmosphere compositionabout 96.5% CO2, about 3.5% N2
Mercury dayside maximumabout 430 C at the equatorial hot poles
Mercury night minimumabout -180 C
Distance from the SunVenus about 0.72 AU, Mercury about 0.39 AU

A seguir: o guia de quando usar ou comparação com alternativas. Abra o Venus Runaway Greenhouse Explorer 3D.

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