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 (9.3 MPa). The Venusian atmosphere supports opaque clouds made 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.
primaryTopic
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 (9.3 MPa). The Venusian atmosphere supports opaque clouds made 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.
has abstract
A atmosfera de Vênus (portuguê ...... para exploração e colonização.
@pt
L'atmosfera di Venere è incred ...... ioni atmosferiche del pianeta.
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La atmósfera de Venus es altam ...... almente 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 ...... met under similar conditions."
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Атмосфера Венеры — газовая обо ...... ля исследования и колонизации.
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لدى كوكب الزهرة غلاف جويّ كثيف ...... في الضغط الجوي ودرجة الحرارة.
@ar
本稿では金星の大気（きんせいのたいき）について述べる。 太陽 ...... 査機マゼランが到着するまでは、金星の地表を調べられなかった。
@ja
金星大氣層是由俄羅斯科學家米哈伊爾·瓦西里耶維奇·羅蒙諾索夫 ...... 離層物質外流的模式與「類似條件下來自彗星彗核的離子尾」類似。
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Wikipage revision ID
742,235,298
avg surface pressure
Caption
Cloud structure in Venus's atmosphere in 1979,
revealed by ultraviolet observations from Pioneer Venus Orbiter
chemical
height
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A atmosfera de Vênus (portuguê ...... tes apenas em pequenos traços.
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L'atmosfera di Venere è incred ...... lettriche di notevole potenza.
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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.
@fr
The atmosphere of Venus is the ...... present only in trace amounts.
@en
Атмосфера Венеры — газовая обо ...... (467 °С), а давление — 93 бар.
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لدى كوكب الزهرة غلاف جويّ كثيف ...... ها موجودة في كميات تافهة فحسب.
@ar
本稿では金星の大気（きんせいのたいき）について述べる。 太陽 ...... 査機マゼランが到着するまでは、金星の地表を調べられなかった。
@ja
金星大氣層是由俄羅斯科學家米哈伊爾·瓦西里耶維奇·羅蒙諾索夫 ...... 大氣層中的氦。因此有人提出可在金星的高層大氣進行探測和殖民。
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label
Atmosfera de Vênus
@pt
Atmosfera di Venere
@it
Atmosphere of Venus
@en
Atmosphère de Vénus
@fr
Atmósfera de Venus
@es
Атмосфера Венеры
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غلاف الزهرة الجوي
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金星の大気
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金星大氣層
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