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  2. Atmosphere of Venus - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Venus

    Components of the induced magnetosphere are shown. Venus is known not to have a magnetic field. [46] [47] The reason for its absence is not at all clear, but it may be related to a reduced intensity of convection in the Venusian mantle. Venus only has an induced magnetosphere formed by the Sun's magnetic field carried by the solar wind. [46]

  3. Magnetosphere - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere

    A rendering of the magnetic field lines of the magnetosphere of the Earth. In astronomy and planetary science, a magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field. [1] [2] It is created by a celestial body with an active interior dynamo.

  4. Category:Magnetospheres - Wikipedia

    en.wikipedia.org/wiki/Category:Magnetospheres

    Download as PDF; Printable version; In other projects ... (2 C, 6 P) Pages in category "Magnetospheres" ... Magnetosphere of Venus

  5. Water on Venus - Wikipedia

    en.wikipedia.org/wiki/Water_on_Venus

    Venus’ cloud data prove that Venus' clouds contain a small amount of water, possibly proving that Venus once had a functioning water cycle. [7] Using image data from Magellan, scientists could fill lowlands of Venus’ surface area with water, leaving only Venusian continents visible.

  6. Magnetosphere of Venus - Wikipedia

    en.wikipedia.org/?title=Magnetosphere_of_Venus&...

    move to sidebar hide. From Wikipedia, the free encyclopedia

  7. Magnetosheath - Wikipedia

    en.wikipedia.org/wiki/Magnetosheath

    The magnetosheath is the region of space between the magnetopause and the bow shock of a planet's magnetosphere.The regularly organized magnetic field generated by the planet becomes weak and irregular in the magnetosheath due to interaction with the incoming solar wind, and is incapable of fully deflecting the highly charged particles.

  8. 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.

  9. Magnetopause - Wikipedia

    en.wikipedia.org/wiki/Magnetopause

    Venus and Mars do not have a planetary magnetic field and do not have a magnetopause. The solar wind interacts with the planet's atmosphere [ 12 ] and a void is created behind the planet. In the case of the Earth's moon and other bodies without a magnetic field or atmosphere, the body's surface interacts with the solar wind and a void is ...