Net Deals Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. Venus (mythology) - Wikipedia

    en.wikipedia.org/wiki/Venus_(mythology)

    Venus ( / ˈviːnəs /) [ a] is a Roman goddess, whose functions encompass love, beauty, desire, sex, fertility, prosperity, and victory. In Roman mythology, she was the ancestor of the Roman people through her son, Aeneas, who survived the fall of Troy and fled to Italy. Julius Caesar claimed her as his ancestor.

  3. Dorothy (Venusian crater) - Wikipedia

    en.wikipedia.org/wiki/Dorothy_(Venusian_crater)

    Dorothy Crater is an impact crater on Venus . The names for small craters on Venus (with a diameter less than 20 km) are chosen from common female names. [2] Dorothy is a Greek first name, and the crater was officially designated by the IAU in 1997. The crater is east of Tamfana Corona, and south of Seoritsu Farra. [3]

  4. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    Here the eight pointed star is the Star of Ishtar, the Babylonian Venus goddess, alongside the solar disk of her brother Shamash and the crescent moon of their father Sin on a boundary stone of Meli-Shipak II, dating to the twelfth century BC. Several hymns praise Inanna in her role as the goddess of the planet Venus.

  5. List of geological features on Venus - Wikipedia

    en.wikipedia.org/wiki/List_of_geological...

    Venus, the second planet from the Sun, is classified as a terrestrial planet. It is sometimes called Earth's "sister planet" due to their similar size, gravity, and bulk composition (Venus is both the closest planet to Earth and the planet closest in size to Earth). The surface of Venus is covered by a dense atmosphere and presents clear ...

  6. Cleopatra (crater) - Wikipedia

    en.wikipedia.org/wiki/Cleopatra_(crater)

    Cleopatra (initially called Cleopatra Patera [2]) is an impact crater on Venus, in Maxwell Montes. Cleopatra is a double-ring impact basin about 100 kilometers (62 mi) in diameter and 2.5 kilometers (1.6 mi) deep. A steep-walled, winding channel a few kilometers wide ( Anuket Vallis) breaks through the rough terrain surrounding the crater rim.

  7. Surface features of Venus - Wikipedia

    en.wikipedia.org/wiki/Surface_features_of_Venus

    Global radar map of the surface 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 ...

  8. Enceladus - Wikipedia

    en.wikipedia.org/wiki/Enceladus

    The rate at which this occurs is dependent on the temperature of the ice: warmer ice is easier to deform than colder, stiffer ice. Viscously relaxed craters tend to have domed floors, or are recognized as craters only by a raised, circular rim. Dunyazad crater is a prime example of a viscously relaxed crater on Enceladus, with a prominent domed ...

  9. Geology of Venus - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Venus

    The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990–1994 Magellan mission, is centered at 180 degrees east longitude. The geology of Venus is the scientific study of the surface, crust, and interior of the planet Venus. Within the Solar System, it is the one nearest to Earth and ...