I'm building a small, naturally inhabited world where usable water is scarce or difficult to access. Is it possible to have a planet with groundwater, ice caps, temporary rivers and lakes, seasonal rains and fog, but no permanent oceans? If so, where might clouds etc come from? Could there be evaporation from shallow, temporary or constantly moving water bodies? Or could significant amounts of moisture be released into the atmosphere directly from the ground, say in steam vents?

  • 5
    $\begingroup$ entirely possible, most of the planets in our own system have no liquid water. DO you mean a world capable of supporting complex life? because then the answer is likely no. $\endgroup$
    – John
    Commented Feb 12, 2017 at 15:02
  • 1
    $\begingroup$ Yes, I intend for the world to support complex life. There would actually bodies of liquid water on the surface, but they would not be permanent. They could dry up or shift according to changing seasons. The intent is that any life would have to either be nomadic and follow the water, or adapt to draw moisture from the ground or the air. $\endgroup$
    – RLoopy
    Commented Feb 12, 2017 at 17:10
  • $\begingroup$ your planet must be tectonically dead, becasue if the ground height varies then oceans will form. $\endgroup$
    – John
    Commented Feb 12, 2017 at 17:12
  • $\begingroup$ LINK LINK So in fiction, it has worked before. $\endgroup$
    – WRX
    Commented Feb 12, 2017 at 18:07
  • $\begingroup$ Mars, about a billion years or so ago, during the transition from the Noachian period, during which it (probably) had an ocean, to its present dry state. en.wikipedia.org/wiki/Mars_ocean_hypothesis Note that Mars today has clouds, and there's some evidence that there may occasionally be liquid water. $\endgroup$
    – jamesqf
    Commented Feb 12, 2017 at 18:08

4 Answers 4


Put the oceans underground

Many moons are theorized to have vast, underground oceans. If you want water to be scarce on the surface, but you need a supply regardless, keep the water in big caverns below the surface.

Cryovolcanic activity - eruptions of water from geysers or "volcanos" - can provide temporary rivers, lakes, and ponds, before the water trickles back down.



TLDR: Have an ocean at the equator to start with, then use a catastrophic event to move your orbit slightly closer to the host star. As a result your planet could be too hot at the equator for liquid water but too high at the poles so all the water runs in rivers from the poles to the equator where it evaporates again.

Naturally this answer is all based on our one and only researchable planet that supported life. Perhaps there are many other ways for life to evolve and a dry surface suits some types too. However on earth the oceans have been pretty pivotal for many reasons but mainly focusing on the process of mixing chemicals - early life wouldn't have had to search for it's food but instead be living in a constantly mixing solution of it.

So all our models suggest that the oceans are pivotal in the origin of life, however this isn't to say your oceans still need to be around. Once life has evolved to walk on land we could have some celestial disaster, one of the outer planets in your solar system moving inwards (possibly as outlined in answers to this question. If the orbit was disrupted so your planet now lay closer to the sun you could find it too hot at the equator to support liquid water but the poles may be just about cool enough.

If your equator was at sea level originally and the poles were not the water which rains down on the poles would run in rivers headed towards the equator, then boil off as they reached it.

This would provide the necessary water cycle but without allowing large bodies of standing water.

However we do have the problem of keeping your life alive. The disaster would be a mass extinction event resulting in:

  • Any fish (and in turn anything that lived on fish) would die.
  • Almost all plant life would die (extremely limited food source now) - desert plants which had already evolved would be best suited to survival, being carried by animals migrating to the poles is the most likely method of dispersion this far.
  • There would be a mass migration towards the poles (interestingly providing reasons for having splits in evolutionary trees).
  • Water would be scarce and most likely result in life with adaptations like the camel's hump and deep roots for plants since water would still be present deep underground.

The world is tidally locked, with mountains at the middle

The same side of the planet always faces the sun, kind of like how we always see the same face of the moon. That means one side of the planet will always be incredibly hot - perhaps too hot for water - and the other will be incredibly cold - making it freeze.

Life can live in the habitable zone in a vast mountain range, kind of like the one on Iapetus - that will prevent large oceans from forming.

From Wikipedia


Apsidal precession

This cycle changes the orbit of the planet over thousands of years. It can cause changes in the world's climate, causing warming - if the water is frozen - or cooling - if the world is too hot.

I'm not an expert, but it seems reasonable for the planet to have a shorter cycle - allowing some water to flow, but preventing the formation of a longterm ocean.


You must log in to answer this question.

Not the answer you're looking for? Browse other questions tagged .