Is the total amount of water on the planet constant?

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Discussion Overview

The discussion centers around the question of whether the total amount of water on Earth is constant. Participants explore various aspects of the water cycle, water loss mechanisms, and the sources of water on the planet, touching on geological, atmospheric, and cosmic factors.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants question the constancy of Earth's water supply, noting that water is lost to space through processes like decomposition and escape of hydrogen.
  • Others argue that while water can be lost, it is also replenished from various sources, including solar system debris and geological processes.
  • A participant mentions that groundwater is part of the water cycle, suggesting that water enters the ground and eventually returns to the oceans.
  • There are discussions about the impact of human activities, such as space exploration, on water loss, with some suggesting that losses from manned missions are negligible.
  • One participant raises the idea of an equilibrium level for water, where the amount lost to space is balanced by the amount received from space.
  • Another participant introduces the concept of water produced from burning hydrocarbons, suggesting that this could contribute to the overall water supply.
  • Some humor is injected into the discussion with a light-hearted comment about water being trapped in the rings of Saturn.

Areas of Agreement / Disagreement

Participants express differing views on whether the total amount of water on Earth is constant. While some suggest that losses and gains may balance out, others highlight the complexities and uncertainties surrounding the water cycle and its interactions with geological and atmospheric processes.

Contextual Notes

Participants note various mechanisms of water loss and gain, but there are unresolved questions regarding the exact quantities involved and the definitions of what constitutes "water" in this context. The discussion also touches on the effects of human activity and natural processes, which may vary in significance.

DeepCut
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Maybe not the correct sub-forum for the question, but is the total amount of water on the planet constant ?

I know the basics of meteorology and the whole sky, sea and land cycle but we put so much water into the land, how does that water get recycled ?

If it is constant then why is it still fresh and pure in streams (streams that don't have industrial dumping!) and rivers ?


Thanks,

DC.
 
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Where do you think the water in streams and rivers comes from?
 
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Some water decomposes (for whatever reasons - high temperatures in volcanoes, radiolysis in high parts of atmosphere), and some of the hydrogen produced is able to escape to space. But we are talking about small amounts, if memory serves me well something like 100kt per year. Oxygen is too heavy for this path.
 
Water can be broken down by natural processes into hydrogen and oxygen, as Borek noted. Hydrogen can escape to space, explaining the mechanism for water loss on earth. While hydrogen and helium are light enough to escape into space, Earth's gravity severely constrains the amount of heavier elements that can escape into space. Earth also vast reserves of water trapped in the mantle and this water is slowly released over time, so the surface supply is continually replenished. Water is also supplied to Earth via solar system debris. While current contributions are difficult to quantify, it is still widely believed they were a major source of Earth's primordial water supply.
 
I know the basics of meteorology and the whole sky, sea and land cycle but we put so much water into the land, how does that water get recycled ?

That's a geology question. When water enters the ground, it sinks until it reaches a layer of nonporous rock, at which point it's called groundwater. Groundwater slowly makes its way downhill through porous rocks and eventually it empties into the ocean.
 
It would depend where you are drawing the line.

If you mean to include the components of water - Hydrogen and Oxygen - then the only losses would be that which escapes the atmosphere into space and that which Man has brought with him on his various explorations off-planet.

Otherwise, it's all here in some form or another.
 
ckirmser said:
It would depend where you are drawing the line.

If you mean to include the components of water - Hydrogen and Oxygen - then the only losses would be that which escapes the atmosphere into space and that which Man has brought with him on his various explorations off-planet.

Otherwise, it's all here in some form or another.

If you're talking about manned spaceflight, then I'd expect the water losses to be slight, because most missions never left Earth orbit. The water would have fallen back into the atmosphere. The moon missions may have left some water on the moon, though.
 
nburns said:
If you're talking about manned spaceflight, then I'd expect the water losses to be slight, because most missions never left Earth orbit. The water would have fallen back into the atmosphere. The moon missions may have left some water on the moon, though.

Not just manned.

I also mean the random water molecules that may have stuck to or in travelers like Voyager, Galileo, Deep Impact, etc.
 
  • #10
Borek said:
Some water decomposes (for whatever reasons - high temperatures in volcanoes, radiolysis in high parts of atmosphere), and some of the hydrogen produced is able to escape to space. But we are talking about small amounts, if memory serves me well something like 100kt per year. Oxygen is too heavy for this path.

The solar wind is mostly hydrogen, it's easy to imagine this material getting caught in, and becoming part of our atmosphere. It seems like the quantity of hydrogen we acquire from the solar wind should be constant (neglecting short term fluctuations). The quantity that we lose from the upper atmosphere should depend on the concentration of hydrogen in the atmosphere. Wouldn't the atmosphere settle to an equilibrium concentration where hydrogen in = hydrogen out? Are we at that level?

Back to the original question about water...
Similar logic should apply. We lose a certain amount of water to space, we get a certain amount of water from space, there should be an equilibrium level where water in = water out. Is there any reason to believe we are not at that level?
 
  • #11
mrspeedybob said:
The solar wind is mostly hydrogen, it's easy to imagine this material getting caught in, and becoming part of our atmosphere. It seems like the quantity of hydrogen we acquire from the solar wind should be constant (neglecting short term fluctuations). The quantity that we lose from the upper atmosphere should depend on the concentration of hydrogen in the atmosphere. Wouldn't the atmosphere settle to an equilibrium concentration where hydrogen in = hydrogen out? Are we at that level?

Interesting point. Simple estimate based on geometry - mass of the Solar wind per year of 4×1016 kg, Earth radius of 6731 km, distance of Earth from Sun of 150×106 km - tells me we could catch around 18 kt per year (which would be mostly hydrogen), compared to 100 kt per year that we loose. The signal is obvious - we are loosing.

Back to the original question about water...
Similar logic should apply. We lose a certain amount of water to space, we get a certain amount of water from space, there should be an equilibrium level where water in = water out. Is there any reason to believe we are not at that level?

Where is the water in space? Or more precisely - where is the oxygen? Solar wind is mostly hydrogen (protons and electrons) as far as I am aware.
 
  • #12
And what about the production of H2O from burning hydrocarbons?
I can't find a number for annual water vapor generation, but according to the EPA, we generated about 5.7 billion tons of CO2 in 2010.
Even if all of that CO2 was generated by burning coal, that would be close to 1 billion tons of water produced per year.
Though according to Chronos's link, there is over a billion times that amount already here.
 
  • #13
  • #14
DeepCut said:
Maybe not the correct sub-forum for the question, but is the total amount of water on the planet constant ?

I know the basics of meteorology and the whole sky, sea and land cycle but we put so much water into the land, how does that water get recycled ?

If it is constant then why is it still fresh and pure in streams (streams that don't have industrial dumping!) and rivers ?


Thanks,

DC.
The water in the streams and oceans evaporates, and this distillation process purifies the water. The contaminants are not, for the most part, able to evaporate with it. It then forms rain droplets in the atmosphere which return to Earth as uncontaminated water. Of course, I'm sure you've heard about acid rain. In this case, acidic species in the atmosphere dissolve in the rain drops and return to earth. That's why it's important to minimize air pollution.

Chet
 
  • #15
Borek said:
Where is the water in space? Or more precisely - where is the oxygen? Solar wind is mostly hydrogen (protons and electrons) as far as I am aware.

"The process of solar-wind hydrogen ions reacting with oxygen in silicate minerals is ubiquitous throughout our solar system, and we can expect that any other star producing a stellar wind with hydrogen ions will be irradiating silicate minerals in dust and on airless bodies in its vicinity, also,"
====
"In no way do we suggest the amount of water from solar wind-irradiated dust was sufficient to form oceans," Ishii said. Still, "because the rainfall of interplanetary dust has been continuous, the cumulative amount of solar-wind–produced water may well have been significant."

http://www.space.com/24422-solar-wind-makes-water-star-dust.html


Abstract

The solar wind (SW), composed of predominantly ∼1-keV H+ ions, produces amorphous rims up to ∼150 nm thick on the surfaces of minerals exposed in space. Silicates with amorphous rims are observed on interplanetary dust particles and on lunar and asteroid soil regolith grains. Implanted H+ may react with oxygen in the minerals to form trace amounts of hydroxyl (−OH) and/or water (H2O). Previous studies have detected hydroxyl in lunar soils, but its chemical state, physical location in the soils, and source(s) are debated. If −OH or H2O is generated in rims on silicate grains, there are important implications for the origins of water in the solar system and other astrophysical environments. By exploiting the high spatial resolution of transmission electron microscopy and valence electron energy-loss spectroscopy, we detect water sealed in vesicles within amorphous rims produced by SW irradiation of silicate mineral grains on the exterior surfaces of interplanetary dust particles. Our findings establish that water is a byproduct of SW space weathering. We conclude, on the basis of the pervasiveness of the SW and silicate materials, that the production of radiolytic SW water on airless bodies is a ubiquitous process throughout the solar system.

http://www.pnas.org/content/early/2014/01/16/1320115111.abstract
 
  • #16
Dotini said:
Our findings establish that water is a byproduct of SW space weathering. We conclude, on the basis of the pervasiveness of the SW and silicate materials, that the production of radiolytic SW water on airless bodies is a ubiquitous process throughout the solar system.

Interesting. Still, I wonder if amount of water that we could get on Earth from such a source now (I mean: in today's Solar system) is large enough to be significant in the context of the thread.
 

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