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  2. Observations and explorations of Venus - Wikipedia

    en.wikipedia.org/wiki/Observations_and...

    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 ...

  3. Never-before seen images of Venus' surface unveiled - AOL

    www.aol.com/lifestyle/never-seen-images-venus...

    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.

  4. Mapping of Venus - Wikipedia

    en.wikipedia.org/wiki/Mapping_of_Venus

    The mapping of Venus refers to the process and results of human description of the geological features of the planet Venus. It involves surface radar images of Venus, construction of geological maps , and the identification of stratigraphic units , volumes of rock with a similar age.

  5. Alpha Regio - Wikipedia

    en.wikipedia.org/wiki/Alpha_Regio

    Alpha Regio is a region of the planet Venus extending for about 1500 kilometers centered at 22°S, 5°E.. It was discovered and named by Richard Goldstein in 1964. [1] The name was approved by the International Astronomical Union's Working Group for Planetary System Nomenclature (IAU/WGPSN) between 1976 and 1979. [2]

  6. Geology of Venus - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Venus

    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.

  7. Volcanism on Venus - Wikipedia

    en.wikipedia.org/wiki/Volcanism_on_Venus

    Locating volcanoes on Venus became possible during the Magellan mission in 1990, which mapped over 95% of the surface of Venus. [32] The surface of Venus is hidden by clouds but surface features can be mapped using synthetic aperture radar. [33] Some images created by this mapping can give a perspective view of the elevation of the surface of ...

  8. Surface features of Venus - Wikipedia

    en.wikipedia.org/wiki/Surface_features_of_Venus

    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.

  9. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    These three features are now the only ones on Venus that do not have female names. [48] First view and first clear 180-degree panorama of Venus's surface as well as any other planet than Earth (1975, Soviet Venera 9 lander). Black-and-white image of barren, black, slate-like rocks against a flat sky. The ground and the probe are the focus.