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<p>Because Venus has no oceans or rain to dissolve the carbon dioxide, large amounts of this <a href="page.php?w=greenhouse_gas">greenhouse gas</a> has remained in the atmosphere. The result is a dense atmosphere about 80 times the pressure of Earth's atmosphere. The planet's lack of a magnetic field and closer proximity to the Sun resulted in the loss of its hydrogen (in the form of water) after two billion years.</p>

<p>Because Mars is small, cold, and lacks a magnetic field, it has retained only a sparse atmosphere. The surface air pressure</p><p>
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