Infinite photos and videos for every Wiki article · Find something interesting to watch in seconds
Infinite photos and videos for every Wiki article · Find something interesting to watch in seconds
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.
Infrared image and artist's concept of the bow shock around R Hydrae
Infrared image and artist's concept of the bow shock around R Hydrae
Artist's rendition of Earth's magnetosphere
Artist's rendition of Earth's magnetosphere
Artist impression of the magnetic field around Tau Boötis b detected in 2020.
Artist impression of the magnetic field around Tau Boötis b detected in 2020.