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Surface of Venus from Venera 13. In 1982, the Soviet Venera 13 sent the first colour image of Venus's surface, revealing an orange-brown flat bedrock surface covered with loose regolith and small flat thin angular rocks, [45] and analysed the X-ray fluorescence of an excavated soil sample. The probe operated for a record 127 minutes on the ...
Soft landing; transmitted from surface for 53 minutes. First pictures from surface. Venera 10 lander: USSR: 25 October 1975: Within a 150 km radius of : Soft landing; transmitted from surface for 65 minutes. Pioneer Venus Multiprobe: USA 9 December 1978
The very first visible-light images of Venus' surface from space have been captured by NASA's Parker Solar Probe, and it could help researchers piece together the mysteries of the distant planet.
Although the surface conditions on Venus are no longer hospitable to any terrestrial-like life that might have formed before this event, there is speculation that life may exist in the upper cloud layers of Venus, 50 km (30 mi) above the surface, where atmospheric conditions are the most Earth-like in the Solar System, [106] with temperatures ...
Venus and the crescent Moon were spotted in the sky above the East Midlands - and stargazers managed to capture photos of the celestial scene.
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The surface of Venus is dominated by geologic features that include volcanoes, large impact craters, and aeolian erosion and sedimentation landforms. Venus has a topography reflecting its single, strong crustal plate, with a unimodal elevation distribution (over 90% of the surface lies within an elevation of -1.0 and 2.5 km) [1] that preserves geologic structures for long periods of time.
The surface of Venus is comparatively flat. When 93% of the topography was mapped by Pioneer Venus Orbiter, scientists found that the total distance from the lowest point to the highest point on the entire surface was about 13 kilometres (8.1 mi), about the same as the vertical distance between the Earth's ocean floor and the higher summits of the Himalayas.