Atmosphere of Venus
The atmosphere of Venus is the layer of gases that surrounds Venus. It is mainly composed of carbon dioxide. Its atmosphere is denser and hotter than the atmosphere of Earth. The temperature at the surface is 740 K (467 °C, 872 °F). The pressure is 93 bar (9.3 MPa).[1] It is composed of carbon dioxide (96.5 %), nitrogen (3.5 %), sulfur dioxide (150 ppm), argon (70 ppm), water vapor (20 ppm), carbon monoxide (17 ppm), helium (12 ppm), hydrogen chloride (0.1–0.6 ppm) and hydrogen fluoride (0.001–0.005 ppm).
Atmosphere Of Venus Media
1761 drawing by Mikhail Lomonosov in his work on the discovery of atmosphere of Venus
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.
References
- ↑ Basilevsky, Alexander T; Head, James W (2003-10-01). "The surface of Venus". Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. ISSN 0034-4885. S2CID 250815558.