Atmosphere of Venus
The atmosphere of Venus is the layer of gases surrounding Venus. It is composed primarily of carbon dioxide and is much denser and hotter than that of Earth. The temperature at the surface is 740 K (467 °C, 872 °F), and the pressure is 93 bar (1,350 psi), roughly the pressure found 900 m (3,000 ft) underwater on Earth. The Venusian atmosphere supports opaque clouds of sulfuric acid, making optical Earth-based and orbital observation of the surface impossible. Information about the topography has been obtained exclusively by radar imaging. Aside from carbon dioxide, the other main component is nitrogen. Other chemical compounds are present only in trace amounts.
1379_Lomonosowa1769 transit of Venus observed from Tahiti1978 in spaceflight2019 in scienceAerospace architectureAkatsuki (spacecraft)Anders PlanmanAshen lightAstronomical filterAstrooceanographyAtmosphereAtmosphere of venusAtmospheric super-rotationCarbon monoxideCarbonyl sulfideClimate of IndiaColonization of VenusColonization of the inner Solar SystemComparative planetary scienceCubeSat UV ExperimentDAVINCIDisulfur dioxideEnVision (spacecraft)Expedition VenusExtraterrestrial atmosphereExtraterrestrial lifeExtraterrestrial liquid waterFloating cities and islands in fictionFred Taylor (physicist)Gas balloonGeology of VenusGeorgy GolitsynGliese 1132 bGliese 581cGreenhouse gasHigh Altitude Venus Operational ConceptHypothetical types of biochemistryIonosphereJAXAJames Hansen
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Atmosphere of Venus
The atmosphere of Venus is the layer of gases surrounding Venus. It is composed primarily of carbon dioxide and is much denser and hotter than that of Earth. The temperature at the surface is 740 K (467 °C, 872 °F), and the pressure is 93 bar (1,350 psi), roughly the pressure found 900 m (3,000 ft) underwater on Earth. The Venusian atmosphere supports opaque clouds of sulfuric acid, making optical Earth-based and orbital observation of the surface impossible. Information about the topography has been obtained exclusively by radar imaging. Aside from carbon dioxide, the other main component is nitrogen. Other chemical compounds are present only in trace amounts.
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A atmosfera de Vênus (portuguê ...... para exploração e colonização.
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Artizarraren atmosfera Lurrare ...... delako ingurune azido batean.
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Atmosfer Venus adalah lapisan ...... nya di Saint Petersburg, Rusia
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Atmosfera Wenus – warstwa gazó ...... maczył refrakcją w atmosferze.
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L'atmosfera de Venus comprèn l ...... a l'exploració i colonització.
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L'atmosfera di Venere è incred ...... stili condizioni atmosferiche.
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La atmosfero de Venuso estis m ...... aj la koloniado de la planedo.
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La atmósfera de Venus es altam ...... lmente de dióxido de carbono.
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L’atmosphère de Vénus a été dé ...... la colonisation de la planète.
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The atmosphere of Venus is the ...... ed the existence of phosphine.
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Cloud structure in Venus's atmosphere in 1979,
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revealed by ultraviolet observations from Pioneer Venus Orbiter
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chemical
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Venus
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A atmosfera de Vênus (portuguê ...... tes apenas em pequenos traços.
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Artizarraren atmosfera Lurrare ...... . Tenperatura hau esterilizazi
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Atmosfer Venus adalah lapisan ...... alam jumlah yang sangat kecil.
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Atmosfera Wenus – warstwa gazó ...... ują się w ilościach śladowych.
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L'atmosfera de Venus comprèn l ...... sents només en petites traces.
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L'atmosfera di Venere è incred ...... lettriche di notevole potenza.
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La atmosfero de Venuso estis m ...... aliaj gasoj aperas nur spure.
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La atmósfera de Venus es altam ...... rte debido a la mayor presión.
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L’atmosphère de Vénus a été dé ...... eulement sous forme de traces.
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The atmosphere of Venus is the ...... present only in trace amounts.
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Artizarraren atmosfera
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Atmosfer Venus
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Atmosfera Wenus
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Atmosfera de Venus
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Atmosfera de Vênus
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Atmosfera di Venere
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Atmosféra Venuše
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Atmosphere of Venus
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Atmosphère de Vénus
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Atmósfera de Venus
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