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  2. Geology of Venus - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Venus

    This implies that Venus lacks convection in its outer core. Convection occurs when there is a large difference in temperature between the inner and outer part of the core, but since Venus has no plate tectonics to let off heat from the mantle, it is possible that outer core convection is being suppressed by a warm mantle.

  3. Atmosphere of Venus - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Venus

    All winds on Venus are ultimately driven by convection. [3] Hot air rises in the equatorial zone, where solar heating is concentrated and flows to the poles. Such an almost-planetwide overturning of the troposphere is called Hadley circulation. [3] However, the meridional air motions are much slower than zonal winds.

  4. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    Venus is the second planet from the Sun. It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth. Venus has by far the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover.

  5. Volcanism on Venus - Wikipedia

    en.wikipedia.org/wiki/Volcanism_on_Venus

    Lightning on Venus may serve as a diagnostic of volcanism or atmospheric convection, so some effort has been devoted to detecting possible lightning on Venus. [18] No lightning has been directly observed, but the most compelling evidence is the very low frequency (VLF) radio emissions recorded beneath the clouds by all four of the Venera ...

  6. Geodynamics of Venus - Wikipedia

    en.wikipedia.org/wiki/Geodynamics_of_Venus

    a transition from mobile lid to stagnant lid convection proposed by Solomatov and Moresi (1996) [12] and a rapid transition from a thin to thick lithosphere proposed by Reese et al. (2007) [ 13 ] The portion of the planet with large rift zones and superposed volcanoes was found to correlate with a low crater density and an unusual number of ...

  7. Hadley cell - Wikipedia

    en.wikipedia.org/wiki/Hadley_cell

    Slower rotating planets or moons, such as on Titan, may support broader Hadley circulations with upward branches and convection closer to the polar regions. Venus, which rotates slowly, may have Hadley cells that extend farther poleward than Earth's, spanning from the equator to high latitudes in each of the northern and southern hemispheres.

  8. Observations and explorations of Venus - Wikipedia

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

    The planet's period of retrograde motion is 20 days on either side of the inferior conjunction. In fact, through a telescope Venus at greatest elongation appears less than half full due to Schröter's effect first noticed in 1793 and shown in 1996 as due to its thick atmosphere. Venus in daylight at 5 p.m. in the southern hemisphere ...

  9. Convection - Wikipedia

    en.wikipedia.org/wiki/Convection

    Convection is often categorised or described by the main effect causing the convective flow; for example, thermal convection. Convection cannot take place in most solids because neither bulk current flows nor significant diffusion of matter can take place. Granular convection is a similar phenomenon in granular material instead of fluids.