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
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 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 through the atmosphere relatively unhindered. The dark spots are clouds silhouetted against the very hot lower atmosphere emitting thermal infrared radiation.
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
Atmosphere of Venus
…lifting gas on Venus in the same way that helium is a lifting gas on Earth, the upper atmosphere has been proposed as a location for both exploration and colonization. Christiaan Huygens was the first to hypothesize the existence of an atmosphere on Venus. In the Book II of Cosmotheoros, published in 1698, he writes…
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.
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