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There are a number of questions on here about possible exotic types of biochemistry on worlds with ammonia or methane oceans. Some of these point out that a plausible pathway would be a reducing atmosphere which has hydrogen released from plants, with animals using that hydrogen to reduce organics back down to methane for energy. A point that comes up in these is that hydrogen will tend to escape from a terrestrial planet, as this chart shows: Chart relating atmospheric gas retention to surface escape velocity of planets

I wonder though, how big a problem is this really? This Jeans Escape diagram illustrates that this leakage only happens in the upper atmosphere, slowly, as the lower levels keep the molecule speeds down in collisions.

Diagram showing escape of high-velocity gas molecules at altitude

There's also this line from the wikipedia article on the subject.

"In 1 billion years, the Sun will be 10% brighter than it is now, making it hot enough for Earth to lose enough hydrogen to space to cause it to lose all of its water"

Earth has not lost its water yet via hydrogen escape, but it one day will, when the upper atmosphere gets much richer in water vapor, exposing more of it to photolysis and hydrogen escape. Right now though, not that much hydrogen is up high enough for this.

Could worlds with ammonia or methane-based life retain hydrogen created by local life long-term in this same manner? Have a slow escape from their upper atmospheres during their long and cold lifetimes until their suns age and grow hotter? Is is plausible to have a terrestrial world where hydrogen was the equivalent of oxygen in its proportions for long stretches of time without the planet drying out? Titan, for example, has an atmosphere of 0.2% Hydrogen despite its small size and still being too warm to hold onto the stuff long-term.

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  • $\begingroup$ It's not clear to me which chemical paths are being used by your equivalent of plants and animals. $\endgroup$
    – L.Dutch
    Commented Jun 21, 2021 at 17:48
  • $\begingroup$ Not sure how relevant that is here, but the ideas put forth in other questions boil down to plants turn methane/ammonia/etc and sunlight into organics and hydrogen, plants use hydrogen to reduce organics into energy and methane. $\endgroup$ Commented Jun 21, 2021 at 17:53

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Could worlds with ammonia or methane-based life retain hydrogen created by local life long-term in this same manner? Have a slow escape from their upper atmospheres during their long and cold lifetimes until their suns age and grow hotter?

This is the wrong question, I believe.

Retention of molecular hydrogen in the upper atmosphere (which is here it will all end up, after all) is absolutely no good for hydrogenotrophs which will largely be living on the planetary surface (or under it).

On earth, one can reasonably expect evaporated water to eventually condense out and return back to the surface, but molecular hydrogen released by whatever biochemical process that escapes into the atmosphere cannot be recycled nearly so easily. High altitude molecular hydrogen may as well have poofed out of existence for all the good that it would do.

The question should be, how can a hydrogen cycle be formed on a world with a less-than-gas-giant-sized gravity well?

Do feel free to ask that, but as a new question rather than an edit to this one ;-)

Titan, for example, has an atmosphere of 0.2% Hydrogen despite its small size and still being too warm to hold onto the stuff long-term.

It is cold, has a massive reserve of hydrocarbons, and has quite a few atmospheric chemical processes that generate hydrogen. Wikipedia lists a few, but it does not list any processes that consume molecular hydrogen and prevent it from simply floating away into space. That ~.1% hydrogen is simply an artefact of a vast amount of hydrogen production.

The presence of large numbers of hydrogenic lifeforms on the surface (or in the atmosphere) would speed up the loss of hydrogen, but whether they'd use it up fast enough to render the world rapidly uninhabitable is again, a question for another day.

I think, though, that in order to have a hydrogen cycle you're probably going to need all the participants to live in an ocean of some kind, something that can slow hydrogen escape fast enough for enough of it to be consumed by hydrogenotrophs. Terrestrial hydrogenotrophs live in places like marine sediments, or your digestive tract, both of which help trap gasses.

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    $\begingroup$ Ehh, is the first half of the answer assuming that this hydrogen will collect itself at the top of atmosphere and at the bottom there will be none/very little of it - like happy hydrogen balloon flying into stratosphere? If yes then it is not what's will happen, if no then maybe some rewording to make it more clear? $\endgroup$
    – MolbOrg
    Commented Sep 15, 2021 at 12:14
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It is just a matter of budgets

How is it I can have any money? I spend so much. But due to a fortuitous set of events, I make it a little bit faster than I spend it. If you spend more money than you take in, you will run out of money. If you take in more than you spend, your wealth will grow.

Consider oxygen. How does it persist in the Earths atmosphere? The entire surface of the earth is coated with reduced carbon compounds that will oxidize and consume the oxygen!

The answer is that photosynthesizers are kicking it out faster than it is consumed. That would work in your world too. And the biochemistry does not have to be that weird - there are plenty of hydrogen generating photosynthesizers in the world now. Your creatures are splitting water and releasing hydrogen faster than it is being consumed or lost to space.


Some people think this was the original form of photosynthesis, from before the Great Oxygenation. It makes sense in a reducing world. Oxygen was the desired molecule, not waste. In a reducing world, if you can make oxygen you can use it to burn reduced molecules in your tissues and release the CO2. In a hydrogen rich reducing world your creatures split H2O, release H2 and hang on to the O2 they make and make energy from ambient reduced molecules in the environment.

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