Editing Venus

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Though [[Mercury]] is closer to the Sun, it doesn't have an atmosphere to retain all the [[heat]]. In contrast, Venus has a dense atmosphere that retains all the heat on the planet. Besides that, due to the volcanic activities the Venusian atmosphere has more [[carbon dioxide]] in it. It is believed that during the formation of the planet, Venus might have had [[ocean]]s, which later boiled and evaporated due to the high temperature.<ref>Ingersoll, Andrew P. "The Runaway Greenhouse: A History Of Water On Venus". Journal of the Atmospheric Sciences 26.6 (1969): 1191-1198. Web. 12 Jan. 2017.</ref> The [[water vapour]] should have [[photodissociation|photodissociated]] into [[hydrogen]] and [[oxygen]]. And the oxygen should have [[oxidation|oxidized]] surface minerals, releasing carbon dioxide, a [[greenhouse gas]] into Venus's atmosphere. The increase in the temperature due to the [[greenhouse effect]] would then evaporate more water into water vapour, another greenhouse gas, and would have enabled a positive feedback on the carbon dioxide-rich atmosphere to form a runaway greenhouse effect that makes Venus, the hottest planet in the solar system.
 
Though [[Mercury]] is closer to the Sun, it doesn't have an atmosphere to retain all the [[heat]]. In contrast, Venus has a dense atmosphere that retains all the heat on the planet. Besides that, due to the volcanic activities the Venusian atmosphere has more [[carbon dioxide]] in it. It is believed that during the formation of the planet, Venus might have had [[ocean]]s, which later boiled and evaporated due to the high temperature.<ref>Ingersoll, Andrew P. "The Runaway Greenhouse: A History Of Water On Venus". Journal of the Atmospheric Sciences 26.6 (1969): 1191-1198. Web. 12 Jan. 2017.</ref> The [[water vapour]] should have [[photodissociation|photodissociated]] into [[hydrogen]] and [[oxygen]]. And the oxygen should have [[oxidation|oxidized]] surface minerals, releasing carbon dioxide, a [[greenhouse gas]] into Venus's atmosphere. The increase in the temperature due to the [[greenhouse effect]] would then evaporate more water into water vapour, another greenhouse gas, and would have enabled a positive feedback on the carbon dioxide-rich atmosphere to form a runaway greenhouse effect that makes Venus, the hottest planet in the solar system.
  
=== How does the Venusian atmosphere survive the solar winds? ===
 
Venus is a massive planet, weighing about 4.868×10<sup>24</sup> kg. Therefore, gravity plays an important role in holding the atmosphere to the planet at the surface level. But due to the slow rotation, the planet has no internal magnetic field. The solar winds, therefore, interact freely with [[ionosphere]] of the planet and strips away lighter elements along with it. This interaction forms an induced magnetosphere with a [[bow shock]], [[magnetosheath]], [[magnetopause]], and a [[magnetotail]]. Though the solar winds interact deep in the atmosphere and strip away a significant part of it, this induced magnetosphere is strong enough to control the interaction during the periods of minimum [[solar activity]]. The primary loss of atmospheric elements and [[plasma]] happens at the magnetotail, with a few [[magnetic reconnections]]. Despite this loss, the induced magnetosphere is still capable of preventing the complete loss of the Venusian atmosphere.
 
 
== References ==
 
== References ==
 
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