<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://apm.bplaced.net/w/index.php?action=history&amp;feed=atom&amp;title=Subsurface_ocean</id>
	<title>Subsurface ocean - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://apm.bplaced.net/w/index.php?action=history&amp;feed=atom&amp;title=Subsurface_ocean"/>
	<link rel="alternate" type="text/html" href="https://apm.bplaced.net/w/index.php?title=Subsurface_ocean&amp;action=history"/>
	<updated>2026-04-20T14:27:20Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.43.0</generator>
	<entry>
		<id>https://apm.bplaced.net/w/index.php?title=Subsurface_ocean&amp;diff=8005&amp;oldid=prev</id>
		<title>Apm: basic version of the page</title>
		<link rel="alternate" type="text/html" href="https://apm.bplaced.net/w/index.php?title=Subsurface_ocean&amp;diff=8005&amp;oldid=prev"/>
		<updated>2020-11-04T12:32:26Z</updated>

		<summary type="html">&lt;p&gt;basic version of the page&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;There are a number of places in our solar system where subsurface oceans are expected. &lt;br /&gt;
In some cases there might be more or less [[cryovolcanism]] present which &lt;br /&gt;
many or may not provide access channels all the way down to the subsurface oceans.&lt;br /&gt;
where a research probe or (even a crewed submarine) may or may not fit through.&lt;br /&gt;
&lt;br /&gt;
== High pressures in these oceans ==&lt;br /&gt;
&lt;br /&gt;
Despite the low gravities of these bodies the great depth of the upper end of these subsurface oceans&lt;br /&gt;
causes a great deal of pressure which may not be easily handelable for some of the bodies.&amp;lt;br&amp;gt;&lt;br /&gt;
{{todo|add some minimum depth and pressure estimations to give some perspective}}&amp;lt;br&amp;gt;&lt;br /&gt;
{{todo|add some temperature estimates too}}&lt;br /&gt;
&lt;br /&gt;
[[cryovolcanism|Cryovlocanic channels and &amp;quot;magma&amp;quot; chambers]] might be easier way accessible than directly melting through through the icy crust.&lt;br /&gt;
Also these would be more interesting for human colonization.&lt;br /&gt;
&lt;br /&gt;
=== APM&amp;#039;s high pressure suitability ===&lt;br /&gt;
&lt;br /&gt;
Note that deep-sea probes built with [[advanced APM]] will be able to handle tremendously higher pressures than what is possible with today&amp;#039;s (2020) technology.&lt;br /&gt;
(See: [[High pressure]]s). It might get to the point where one needs to think about avoiding crystal structures of the probe being crushed rather than rather than internal voids being crushed.&lt;br /&gt;
There is much less heat in many of the bodies of interest than when going down in depth on Earth.&lt;br /&gt;
And extreme heat is the bigger problem for [[advanced AP systems]].&lt;br /&gt;
Also there is massive temperature equilibration in an open body of water. &lt;br /&gt;
At the depth of the Mariana Trench but under land it is way hotter than just 4°C due to the [https://en.wikipedia.org/wiki/Geothermal_gradient geothermal gradient] that is not present in water.&lt;br /&gt;
&lt;br /&gt;
== List of bodies with potential subsurface oceans ==&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;mars&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
* Well, not an ocean but some &amp;quot;small&amp;quot; lakes under thick ice sheets have been confirmed.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Asteroid belt:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
* Ceres -- it does not visually obviously look like it but there are wight salt spots (and a strange young mountain) proving [[cryovolcanism]]&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Moons of Jupiter:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
* Europa --  Probably the best bet to find one. It has by far the youngest surface. It literally looks like ice on an ocean.&lt;br /&gt;
* Ganymede -- visually its in-between Europa and Kallisto&lt;br /&gt;
* Kallisto -- It&amp;#039;s quite heavily crated and does not visually look like it&amp;#039;s harbouring a subsurface ocean &amp;lt;br&amp;gt;{{todo|find out what&amp;#039;s the water ice to siclicate rock ratio on Kallistos surface}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Moons of Saturn:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
* Titan -- it visually doe not look like it but instruments tell otherwise {{wiki-todo|further investigate knowns about titans hypothetical subsurface ocean}}&lt;br /&gt;
* Enceladus -- huge water ice plumes from cracks confirmed&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Moons of Neptune:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
* Triton -- gysirs confirmed.&lt;br /&gt;
&lt;br /&gt;
* Pluto and Charon? -- It seems like there is some large scale some nitrogen ice convection going. There may be some cryocolcanism involved. We don&amp;#039;t know.&lt;/div&gt;</summary>
		<author><name>Apm</name></author>
	</entry>
</feed>