Impressão artística da radiação estelar a passar através da atmosfera de um exoplaneta. Parte da radiação estelar é absorvida na atmosfera por moléculas de água, óxido de titânio ou sódio, enquanto outras partes são dispersas ou passam através da atmosfera praticamente sem interagir com ela. (Crédito: ESO/M. Kornmesser)
The results, which will soon be published in three papers with the participation of several Instituto de Astrofísica e Ciências do Espaço (IA) researchers, illustrate this instrument’s capabilities to characterize exoplanetary atmospheres.
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