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	<title>Differences between Earth and Venus - Revision history</title>
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		<summary type="html">&lt;p&gt;Article written and Venn diagram created.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Earth vs. Venus ==&lt;br /&gt;
Venus is often called Earth&amp;#039;s &amp;quot;sister planet&amp;quot; due to their similar size, mass, density, and composition.&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt; Both are terrestrial planets that formed around the same time, approximately 4.5 billion years ago.&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; However, despite these foundational similarities, the two worlds evolved into vastly different environments. Earth supports a wide diversity of life, while Venus has a hostile surface, making it the hottest planet in the solar system.&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref5&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Comparison Table ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Category !! Earth !! Venus&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Diameter&amp;#039;&amp;#039;&amp;#039; || 12,756 km (7,926 mi) || 12,104 km (7,521 mi)&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Mass&amp;#039;&amp;#039;&amp;#039; || 5.97 x 10²⁴ kg || 4.87 x 10²⁴ kg&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;Orbital Period (Year)&amp;#039;&amp;#039;&amp;#039; || 365.25 Earth days || 224.7 Earth days&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;Rotational Period (Sidereal Day)&amp;#039;&amp;#039;&amp;#039; || 23 hours, 56 minutes || 243 Earth days (retrograde)&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;Average Surface Temperature&amp;#039;&amp;#039;&amp;#039; || 15°C (59°F) || 464°C (867°F)&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Atmospheric Composition&amp;#039;&amp;#039;&amp;#039; || 78% Nitrogen, 21% Oxygen, 1% Other || 96.5% Carbon Dioxide, 3.5% Nitrogen&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Surface Pressure&amp;#039;&amp;#039;&amp;#039; || 1 bar || 92-93 bars&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Magnetic Field&amp;#039;&amp;#039;&amp;#039; || Substantial, internally generated || Very weak, induced by solar wind&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Venn_diagram_Differences_between_Earth_versus_Venus_comparison.png|thumb|center|800px|alt=Venn diagram for Differences between Earth and Venus|Venn diagram comparing Differences between Earth and Venus]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
The most significant difference between Earth and Venus is their atmospheres. Venus possesses a thick, dense atmosphere composed almost entirely of carbon dioxide, with clouds of sulfuric acid. This creates an extreme greenhouse effect, trapping heat and raising the planet&amp;#039;s surface temperature to an average of 464°C (867°F). The atmospheric pressure at the surface of Venus is over 90 times that of Earth&amp;#039;s, comparable to the pressure deep in Earth&amp;#039;s oceans. In contrast, Earth&amp;#039;s atmosphere is primarily nitrogen and oxygen, which provides a more moderate greenhouse effect, allowing for stable temperatures and liquid water.&lt;br /&gt;
&lt;br /&gt;
=== Surface&amp;lt;ref name=&amp;quot;ref5&amp;quot; /&amp;gt; and Geology ===&lt;br /&gt;
Due to its extreme surface conditions, Venus lacks liquid water. Its surface&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; is a dry, rocky landscape dominated by volcanic features. While both planets have varied terrains with mountains and plains, Venus does not show evidence of the plate tectonics that shape Earth&amp;#039;s surface. Instead, volcanic activity appears to be the primary agent of geological change on Venus. The surface of Venus is also considered relatively young, having undergone a resurfacing event an estimated 300 to 600 million years ago.&lt;br /&gt;
&lt;br /&gt;
=== Rotation and Orbit ===&lt;br /&gt;
Venus&amp;#039;s rotation is unusual. It rotates on its axis very slowly, taking 243 Earth days to complete one rotation. This rotation&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; is also retrograde, meaning it spins in the opposite direction to its orbit around the Sun and in the opposite direction of most other planets. A Venusian day&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; is longer than its year of 225 Earth days. This slow rotation is a contributing factor to its lack of a significant, internally generated magnetic field like Earth&amp;#039;s. Instead, Venus has a weak induced magnetic field created by the interaction of the solar wind with its ionosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&amp;lt;references&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref1&amp;quot;&amp;gt;[https://sci.esa.int/web/venus-express/-/34067-venus-vs-earth &amp;quot;esa.int&amp;quot;]. Retrieved December 12, 2025.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref2&amp;quot;&amp;gt;[https://www.britannica.com/science/How-Big-Is-Venus &amp;quot;britannica.com&amp;quot;]. Retrieved December 12, 2025.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref3&amp;quot;&amp;gt;[https://global.jaxa.jp/countdown/f17/overview/venus_e.html &amp;quot;jaxa.jp&amp;quot;]. Retrieved December 12, 2025.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref4&amp;quot;&amp;gt;[https://www.universetoday.com/articles/temperature-of-venus &amp;quot;universetoday.com&amp;quot;]. Retrieved December 12, 2025.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref5&amp;quot;&amp;gt;[https://medium.com/illuminations-mirror/earth-vs-venus-key-differences-between-two-sister-planets-5964adf90916 &amp;quot;medium.com&amp;quot;]. Retrieved December 12, 2025.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;/references&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Comparisons]]&lt;/div&gt;</summary>
		<author><name>Dwg</name></author>
		
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