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	<title>Lineae - Revision history</title>
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	<updated>2026-04-05T01:47:38Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://wikimd.com/index.php?title=Lineae&amp;diff=5836505&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
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		<updated>2024-05-28T02:39:06Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[File:PIA00295_Europa_dark_bands.jpg|PIA00295 Europa dark bands|thumb]] &amp;#039;&amp;#039;&amp;#039;Lineae&amp;#039;&amp;#039;&amp;#039; are long, narrow, dark markings or lines found on the surface of certain celestial bodies, particularly on [[Mars]] and [[Europa (moon)|Europa]]. These features are of significant interest in the field of [[planetary science]] and [[astrogeology]].&lt;br /&gt;
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== Characteristics ==&lt;br /&gt;
Lineae are typically characterized by their linear appearance, which can extend for hundreds or even thousands of kilometers. They are often darker than the surrounding terrain, making them easily distinguishable in images captured by spacecraft.&lt;br /&gt;
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=== Mars ===&lt;br /&gt;
On [[Mars]], lineae are often associated with [[slope streaks]] and [[recurring slope lineae]] (RSL). These features are thought to be related to the seasonal flow of briny water or dry granular flows. The study of Martian lineae provides insights into the planet&amp;#039;s [[geology]], [[climate]], and potential for [[life on Mars|habitability]].&lt;br /&gt;
&lt;br /&gt;
=== Europa ===&lt;br /&gt;
On [[Europa (moon)|Europa]], one of [[Jupiter]]&amp;#039;s moons, lineae are believed to be caused by the cracking and shifting of the moon&amp;#039;s icy crust. These features are indicative of the dynamic processes occurring beneath the surface, possibly involving a subsurface [[ocean]] of liquid water. The presence of lineae on Europa is a key factor in the moon&amp;#039;s potential to support [[extraterrestrial life]].&lt;br /&gt;
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== Formation ==&lt;br /&gt;
The formation of lineae varies depending on the celestial body. On Mars, they may form due to the flow of liquid water or dry granular material down slopes. On Europa, they are likely formed by tectonic processes, where the icy crust is pulled apart and new material from below fills the gaps.&lt;br /&gt;
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== Significance ==&lt;br /&gt;
The study of lineae is crucial for understanding the geological history and current activity of celestial bodies. On Mars, they provide evidence of past or present water activity, which is essential for assessing the planet&amp;#039;s habitability. On Europa, they suggest the presence of a subsurface ocean, which could harbor life.&lt;br /&gt;
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== Related Pages ==&lt;br /&gt;
* [[Mars]]&lt;br /&gt;
* [[Europa (moon)]]&lt;br /&gt;
* [[Slope streaks]]&lt;br /&gt;
* [[Recurring slope lineae]]&lt;br /&gt;
* [[Planetary science]]&lt;br /&gt;
* [[Astrogeology]]&lt;br /&gt;
* [[Extraterrestrial life]]&lt;br /&gt;
&lt;br /&gt;
== See Also ==&lt;br /&gt;
* [[Geology of Mars]]&lt;br /&gt;
* [[Habitability of natural satellites]]&lt;br /&gt;
* [[Astrobiology]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Planetary science]]&lt;br /&gt;
[[Category:Astrogeology]]&lt;br /&gt;
[[Category:Mars]]&lt;br /&gt;
[[Category:Europa (moon)]]&lt;br /&gt;
[[Category:Geological features]]&lt;br /&gt;
&lt;br /&gt;
{{Planetary-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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