WikiVisually
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
WikiVisually
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
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Colonization of Venus
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The colonization of Venus is the proposed process of establishing human settlements on the planet Venus. Due to the planet's extremely hostile surface environment, proposals for settling Venus focus o
Artist's rendering of a crewed floating outpost on Venus of NASA's High Altitude Venus Operational Concept (HAVOC)
Artist's rendering of a crewed floating outpost on Venus of NASA's High Altitude Venus Operational Concept (HAVOC)
The surface of Venus is completely covered by clouds which prevent most heat from escaping.
The surface of Venus is completely covered by clouds which prevent most heat from escaping.
Artist's conception of a terraformed Venus. The cloud formations are depicted assuming the planet's rotation has not been sped up.
Artist's conception of a terraformed Venus. The cloud formations are depicted assuming the planet's rotation has not been sped up.
MESSENGER Venus 630 nm stretch
MESSENGER Venus 630 nm stretch
Atmosphere of Venus
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The atmosphere of Venus is the very dense layer of gases surrounding the planet Venus. Venus's atmosphere is composed of 96.5% carbon dioxide and 3.5% nitrogen, with other chemical compounds present o
1761 drawing by Mikhail Lomonosov in his work on the discovery of atmosphere of Venus
1761 drawing by Mikhail Lomonosov in his work on the discovery of atmosphere of Venus
Composite image of the polar vortex of Venus in strong red (red image is an infrared view of hot high clouds and the grey image is an ultra-violet vie
Composite image of the polar vortex of Venus in strong red (red image is an infrared view of hot high clouds and the grey image is an ultra-violet view of lower clouds)
Meridional (north-south) component of the atmospheric circulation in the atmosphere of Venus. Note that the meridional circulation is much lower than
Meridional (north-south) component of the atmospheric circulation in the atmosphere of Venus. Note that the meridional circulation is much lower than the zonal circulation, which transports heat between the day and night sides of the planet
False colour near-infrared (2.3 μm) image of the deep atmosphere of Venus obtained by Galileo, red areas are signatures of the hot surface radiating t
False colour near-infrared (2.3 μm) image of the deep atmosphere of Venus obtained by Galileo, red areas are signatures of the hot surface radiating through the atmosphere relatively unhindered. The dark spots are clouds silhouetted against the very hot lower atmosphere emitting thermal infrared radiation.