Oxygen formation in Earth water

AI Thread Summary
The discussion centers on the origins of water and oxygen on Earth, particularly how water could exist without free oxygen. It highlights that cyanobacteria, which are photosynthetic microbes, played a crucial role in oxygenating the atmosphere through photosynthesis, significantly altering Earth's environment. Stromatolites, formed by cyanobacteria, are noted for their contribution to this process. The early Earth’s atmosphere was primarily composed of gases like hydrogen, methane, and ammonia, with water likely locked in the crust during formation. Volcanic activity is believed to have released water vapor, leading to ocean formation. Theories about the origins of Earth's water suggest it may have accreted alongside the planet rather than being delivered by comets or meteorites. The conversation also touches on the complexity of early atmospheric conditions and the interplay between geological and biological processes in shaping the planet's environment.
cookiemonster13
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I always wondered why they say water and photons created the first microbes which later evolved and produced oxygen which filled our oceans and atmosphere. So how could have water existed without oxygen? I tried to look up and came up with different explanations, but it doesn't make sense.
 
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cookiemonster13 said:
I always wondered why they say water and photons created the first microbes which later evolved and produced oxygen which filled our oceans and atmosphere. So how could have water existed without oxygen? I tried to look up and came up with different explanations, but it doesn't make sense.
You need to read about stromatolites.

from the link below

Bacteria, including the photosynthetic cyanobacteria, were the only form of life on Earth for the first 2 billion years that life existed on Earth. Stromatolites are layered mounds, columns, and sheet-like sedimentary rocks. They were originally formed by the growth of layer upon layer of cyanobacteria, a single-celled photosynthesizing microbe that lives today in a wide range of environments ranging from the shallow shelf to lakes, rivers, and even soils. Cyanobacteria are prokaryotic cells (the simplest form of modern carbon-based life) in that they lack a DNA-packaging nucleus.

Although simple, cyanobacteria were ultimately responsible for one of the most important "global changes" that the Earth has undergone. Being photosynthetic, cyanobacteria produce oxygen as a by-product. Photosynthesis is the only major source of free oxygen gas in the atmosphere. As stromatolites became more common 2.5 billion years ago, they gradually changed the Earth's atmosphere from a carbon dioxide-rich mixture to the present-day oxygen-rich atmosphere. This major change paved the way for the next evolutionary step, the appearance of life based on the eukaryotic cell (cell with a nucleus).

http://www.indiana.edu/~geol105b/images/gaia_chapter_10/stromatolites.htm
 
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Totally agree with that. But they needed water to survive. Hence H2O, then how? o.o
idk if I am wrong here..
 
cookiemonster13 said:
Totally agree with that. But they needed water to survive. Hence H2O, then how? o.o
idk if I am wrong here..
That appears to be something that is unknown, there are some theories. I will do more searching for you later today, I was unable to come up with much earlier, just the usual theories, comets, asteroids... That may be the best we have at this time.

http://www.livescience.com/33391-where-did-water-come-from.html
 
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cookiemonster13 said:
I always wondered why they say water and photons created the first microbes which later evolved and produced oxygen which filled our oceans and atmosphere. So how could have water existed without oxygen?

I think you will find that the microbes just added the oxygen content to the atmosphere as stated in that link @Evo gave.
There's no reason to suggest that the microbes existed BEFORE the oceans, which is what you are suggesting

So do you have any links to back up your "they say" claim ?Dave
 
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Evo said:
That appears to be something that is unknown, there are some theories. I will do more searching for you later today, I was unable to come up with much earlier, just the usual theories, comets, asteroids... That may be the best we have at this time.

http://www.livescience.com/33391-where-did-water-come-from.html
Thanks.. :)
 
davenn said:
I think you will find that the microbes just added the oxygen content to the atmosphere as stated in that link @Evo gave.
There's no reason to suggest that the microbes existed BEFORE the oceans, which is what you are suggesting

So do you have any links to back up your "they say" claim ?Dave
Hi sup? I don't really remember. I watched some documentaries and googled up some stuffs. I'll try to look for that and send it to you.
 
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no prob's :smile:

it's just a really good idea to give links (reliable ones) to claims
you will find that "they say" doesn't really cut the mustard on the forumand btw ... welcome to PFDave
 
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th
davenn said:
no prob's :smile:

it's just a really good idea to give links ( reliable ones) to claims
you will find that "they say" doesn't really cut the mustard on the forumand btw ... welcome to PFDave
thanks bro
 
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  • #10
The role of stromatolites in the oxygenation of Earth is a "yes, but..." story. I have a couple hundred papers that show the complexity of the problem. I was, and am, more concerned with astrobiology and the origin of life and my experience in molecular paleontology is with a Jurassic and younger earth. I'll post a few of the papers now. The first has a nice chart showing some major biogeochemical changes in the early earth. Significant is that there is a huge burst in C-13 associated with stromatolites.

Global Biogeochemical Changes at Both Ends of the Proterozoic: Insights from Phosphorites
ASTROBIOLOGY Volume 10, Number 2, 2010 a Mary Ann Liebert, Inc. DOI: 10.1089=ast.2009.0360

Availability of O2 and H2O2 on Pre-Photosynthetic Earth
ASTROBIOLOGY Volume 11, Number 4, 2011 a Mary Ann Liebert, Inc. DOI: 10.1089/ast.2010.0572

Stromatolites in the *3400 Ma Strelley Pool Formation, Western Australia: Examining Biogenicity
from the Macro- to the Nano-Scale
ASTROBIOLOGY Volume 10, Number 4, 2010 a Mary Ann Liebert, Inc. DOI: 10.1089=ast.2009.0423

The case for a Neoproterozoic Oxygenation Event: Geochemical evidence and biological consequences
http://www.geosociety.org/gsatoday/archive/21/3/article/i105

The Proterozoic Record of Eukaryotes
http://paleobiol.geoscienceworld.org/content/41/4/610.abstract?ijkey=171be971757c6becfb61c21509908b70a1215f50&keytype2=tf_ipsecsha

Tropical laterites, life on land, and the history of atmospheric oxygen in the Paleoproterozoic
http://geology.gsapubs.org/content/30/6/491.full.pdf

Were kinetics of Archean calcium carbonate precipitation related to oxygen concentration?
http://geology.gsapubs.org/content/24/2/119.full.pdf+html

Oxygen in the Precambrian atmosphere: An evaluation of the geological evidence
http://geology.gsapubs.org/content/10/3/141.full.pdf+html

This is a decent start, I think.

 
  • #11
https://arxiv.org/pdf/1011.2710v1.pdf
Formation of early water oceans on rocky planets

Lindy E-T, the author of that paper, showed that enough water could be carried in the primordial dust and survived the accretionary phases such that the Earth had enough water in its earliest stages to account for the water that is now here. Asteroids, meteorites and comets aren't needed to account for the original ocean volume.
Occam's origin of the Moon Nature Geoscience 6, 996–998 (2013) doi:10.1038/ngeo2026
"Following almost three decades of some certainty over how the Moon was formed, new geochemical measurements have thrown the planetary science community back into doubt. We are either modelling the wrong process, or modelling the process wrong." Should ()new theories of the moon's origin become a new thread, I'll post some links.

I put there for the cautionary advice that applies to all systems modelling, especially when many proxies are used in place of the reaL deal.
 
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  • #12
@CapnGranite
Astrobiology seems to behind a paywall, specifically the first article: DOI: 10.1089=ast.2009.0360
Since there are several of these, $US 51.00 for each one. Geosociety.org papers - same thing.

@D H - are there any open access "seminal" papers on oxygenation of the Early atmosphere, that are comparable? I am assuming you can see these.
 
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  • #13
I think what cookiemonster is asking is simply "where did the first water on Earth come from? Perhaps we should just stick with that question. :smile: @CapnGranite I think a couple of papers you attempted to link might have more detail than the article I linked.
 
  • #14
http://news.nationalgeographic.com/news/2014/10/141030-starstruck-earth-water-origin-vesta-science/
Mystery of Earth's Water Origin Solved
Instead of arriving later by comet impact, Earth's waters have likely existed since our planet's birth.
"The study shows that Earth's water most likely accreted at the same time as the rock," said Marschall.

This is the only unlocked paper/article I have on the computer.

While this isn't open-access, Science magazine is in many libraries. This is one of the most recent papers on the origin of the Earth's water.
http://science.sciencemag.org/content/sci/346/6209/623.full.pdf
Early accretion of water in the inner solar system from a carbonaceous chondrite–like source
ABSTRACT:
Determining the origin of water and the timing of its accretion within the inner solar system is important for understanding the dynamics of planet formation. The timing of water accretion to the inner solar system also has implications for how and when life emerged on Earth. We report in situ measurements of the hydrogen isotopic composition of the mineral apatite in eucrite meteorites, whose parent body is the main-belt asteroid 4 Vesta. These measurements sample one of the oldest hydrogen reservoirs in the solar system and show that Vesta contains the same hydrogen isotopic composition as that of carbonaceous chondrites. Taking into account the old ages of eucrite meteorites and their similarity to Earth’s isotopic ratios of hydrogen, carbon, and nitrogen, we demonstrate that these volatiles could have been added early to Earth, rather than gained during a late accretion event.
"Our findings cannot preclude a late addition of water for Earth with a carbonaceous chondrite–like D/H, but the observation indicates that a late addition of water is not necessary"
 
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  • #15
CapnGranite said:
http://news.nationalgeographic.com/news/2014/10/141030-starstruck-earth-water-origin-vesta-science/
Mystery of Earth's Water Origin Solved
Instead of arriving later by comet impact, Earth's waters have likely existed since our planet's birth.
"The study shows that Earth's water most likely accreted at the same time as the rock," said Marschall.
Thank you. I think this probably won't satisfy CookieMonster's question of how water could have formed (H2O) if there was no oxygen present to create the water. Was there oxygen present when the Earth formed and the water was created or was that not necessary, this is where it really gets out of my realm of armchair reading.

I know one of you knows the answer.
 
  • #16
The water existed as ice before the Earth was formed.

http://www.cosmos.esa.int/documents...oloS.pdf/6e43745b-f365-4c8c-811c-e679c5fd1a54
Interstellar Water Ice Formation: A laboratory perspective

That was in
http://www.cosmos.esa.int/web/herschel/water-in-the-universe-from-clouds-to-oceans
WATER IN THE UNIVERSE: FROM CLOUDS TO OCEANS
The conference covered all astrophysical aspects of water, including the water trail, from the formation of water in molecular clouds to water on planetary bodies, including in our own solar system; water as a probe of physics and and chemistry; and water in nearby to water in extragalactic and high redshift sources.
 
  • #17
Sorry, I can't make any sense of this. Do I understand that the question is why/how oxygen atoms were originally present on Earth as it emerged from the condensing solar system cloud?

Of course there were oxygen atoms (almost all of them chemically combined of course), lots and lots of them. Our parent supernova(e) plus its parent sun(s) produced elements eventually up to the transuranics, including Pm and Tc, though not all of them in the same concentrations and not all of them lasting long. Oxygen, Si, and Fe were among the commonest (surprise) and in the eventual settling out of various substances, Si and O wound up in the crust in huge proportions. However, there also were fair amounts of H, S, Li, Na, C and the whole alphabet soup, enough that only traces of free O2 or O3 ever existed, and that transiently when it did. But water was fairly plentiful and so were various other hydroxides and hydroxyl compounds. We call such things oceans, right?

The problem was not where the O atoms (in compounds) came from; they were there. The problem was where the free oxygen came from, because O2 is so reactive. That was where photosynthesis came in, and after it had been going for a while, given the plentiful quantities of CO2 and H2O to work on, we wound up with lots of O2.

So OK, I'm stupid; what's the mystery?
 
  • #18
It might help to add, that if we look at any sort of chemical mess in a mud-and-rock ball such as early Earth, with all sorts of compounds being mixed up in heat and cold and radiation and what not (no life yet!) the range of reactions that we might expect, and the mutual co-precipitations and crystallisations would ensure that all sorts of compounds would form, change and re-form, always favouring the most stable forms under reigning conditions and equilibria. Hence plenty of H2O, NH3, CO2, SiO2 and so on.

Right?
 
  • #19
This explanation about life force generating free oxygen ignores the fact that more than 90% of the CO2 on our planet is locked up in rocks by nonliving force. All that locked up CO2 was in the atmosphere early on in Earth's history. The rocks have the truth and it has not yet been discovered by science so a little humility, please.
 
  • #20
Depending on the redox conditions as the Earth was in that early stage of differentiation and degassing, chemical species were forming and disappearing. Jon Richfield has is correct, as I see it, but it was a bit more complex. I'm not so sure that O2 increases in the atmosphere came from the rise of bacteria alone. After the initial, and probable high S and CO2 period, there is evidence that degassing and reactions shifted that environment to one favorable for stable O2. At the same time, stromatolites and free-floating bacteria added to the atmospheric oxygen.
There is a a lack of humility in saying " All that locked up CO2 was in the atmosphere early on in Earth's history."
 
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  • #21
CapnGranite said:
... it was a bit more complex. ...
There is a a lack of humility in saying " All that locked up CO2 was in the atmosphere early on in Earth's history."
Whenever we deal with processes on planetary scales, you can be pretty darn certain that it will be more complex than anyone had guessed.
I suspect that we have about as much CO2 as Venus, only ours is mainly in rock that would not have been able to hold onto its CO2 at Venusian temperatures.

But bottom line remains: Earth had plenty of oxygen from earliest days on.
 
  • #22
Well let's not nitpick-I agree photosynthesis has added O2 to the atmosphere. My point is free oxygen has always been in the atmosphere at about 10E18kg or so. The fact that much more CO2 was in the early atmosphere(CO2 now in rocks)and dwarfs the other gases. This is not known and I just want you to do a calculation of how much CO2 rocks like calcite, dolomite and other rocks have absorbed from the early atmosphere. Not rocket science in any way.
 
  • #23
Understanding the Carbon Earth is not rocket science, for sure. It's also best left to another thread. I'm not sure calculating "how much CO2 rocks like..." is a particularly fundable project, or insightful.
 
  • #24
The two gases are linked and very important to get right. As current state of art theory says the free oxygen came from CO2-right? The rub is that there is way too much CO2 locked up in rocks to be covered by the photosynthesis theory. The Bulk of the original CO2 had to have been locked away in rocks before any living thing would have had an environment to survive in. And photosynthesis generates hydrocarbons not calcite.
 
  • #25
a lot of ocean flora end up precipitating calcite or other carbonates
 
  • #26
Well OK if life force did the job. The job still had to be done before the environment was fit for life capable of doing photosynthesis or before the job of freeing oxygen can be done. Now we have a chicken/egg problem as in which comes first. Is there a life form that can live in CO2 atmospheres?
 
  • #27
jim meyer said:
Well OK if life force did the job. The job still had to be done before the environment was fit for life capable of doing photosynthesis or before the job of freeing oxygen can be done. Now we have a chicken/egg problem as in which comes first. Is there a life form that can live in CO2 atmospheres?

Bacteria.

My take on this ordeal: Prior to ocean formation the atmosphere had been mainly hydrogen, helium, methane, and ammonia. It is now believed that much of the water and rock had been locked into the crust, at the same time, during formation and that a small contribution was made by water-rich meteorite impacts. A lot of volcanic activity released water vapor into the atmosphere, along with carbon dioxide; which, then formed heavy clouds over the Earth that rained for a long time- eventually, forming the ocean. Water came first, not oxygen.
 
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  • #28
Except that I think the evidence is increasing for the water-rich meteorite impacts not being necessary for the primary ocean formation. The volcanic activity suggests that deeper-seated water was brought to the surface by tectonic activity and the volcanism. The later bombardment by water-rich meteorites added to the water volume. I suppose there are two camps regarding the origin of the oceans, water-enstatite grains along with other mineral material, accreting to for the Earth and the group that invokes the bombardment as being the primary source of water. Since around 2011 and up to today, everybody I know and have spoken to favors the first model.
 
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  • #29
CapnGranite said:
Except that I think the evidence is increasing for the water-rich meteorite impacts not being necessary for the primary ocean formation. The volcanic activity suggests that deeper-seated water was brought to the surface by tectonic activity and the volcanism. The later bombardment by water-rich meteorites added to the water volume. I suppose there are two camps regarding the origin of the oceans, water-enstatite grains along with other mineral material, accreting to for the Earth and the group that invokes the bombardment as being the primary source of water. Since around 2011 and up to today, everybody I know and have spoken to favors the first model.

I do think you are right. It may be more right to say that water was locked into the crust as material accreted and later impacts may have contributed some.

Still, this explanation doesn't satisfy me. Something is off. Looking at all the advancements we have made (look at what we can describe about the universe) and comparing it to how little we can explain about the formation of the early Earth makes me uncomfortable.
 
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  • #30
I am happiest when I have a rock to crack open with my rock hammer. In the past, in oil exploration, the drilling sample and cores from an exact depth were what was "real". The seismic sections that we relied on to select the spot to drill gave us data that we manipulated to create the profile. The validation of the seismic data came with a real sample from that data. In recent years I've been involved in about a dozen diamond anvil cell experiments. The results are what they are, but I feel a bit uneasy about extrapolating the results from that tiny universe to the interior of planets. The work that the consortium that is the Deep Carbon Observatory has revealed an Earth interior that would have been pure science fiction in the late '60s, when I first got interested in that.

Something that keeps things in perspective is the notion of multiple-working hypotheses. Even though carrying along old ideas is getting cumbersome, I don't reject them outright for the most part. I run with what works until there is a problem. Sometimes looking back at older ideas can provide insight. If I'm not editing a paper, I try to read 4 papers a day out of the 20-50 I download 6 days a week. I mention all this to show how hard it is to synthesize all the information into something coherent and insightful in a platform like this forum.
 
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  • #31
CapnGranite said:
I am happiest when I have a rock to crack open with my rock hammer. In the past, in oil exploration, the drilling sample and cores from an exact depth were what was "real". The seismic sections that we relied on to select the spot to drill gave us data that we manipulated to create the profile. The validation of the seismic data came with a real sample from that data. In recent years I've been involved in about a dozen diamond anvil cell experiments. The results are what they are, but I feel a bit uneasy about extrapolating the results from that tiny universe to the interior of planets. The work that the consortium that is the Deep Carbon Observatory has revealed an Earth interior that would have been pure science fiction in the late '60s, when I first got interested in that.

Something that keeps things in perspective is the notion of multiple-working hypotheses. Even though carrying along old ideas is getting cumbersome, I don't reject them outright for the most part. I run with what works until there is a problem. Sometimes looking back at older ideas can provide insight. If I'm not editing a paper, I try to read 4 papers a day out of the 20-50 I download 6 days a week. I mention all this to show how hard it is to synthesize all the information into something coherent and insightful in a platform like this forum.

That sounds like a fun career!
 
  • #32
cookiemonster13 said:
Totally agree with that. But they needed water to survive. Hence H2O, then how? o.o
idk if I am wrong here..

No, there are bacteria, called anaerobes, that can live in the absence of O2. In fact, there are anaerobes, called obligate anaerobes, that cannot live in the presence of oxygen, i.e. it's a poison to them. The story, as related to me by several geology books, is that the Earth's early atmosphere was free of O2 and all bacteria were anaerobes. When blue-green algae, which are really a species of bacteria, evolved they could take light as an energy source to split water (That takes a lot of energy, BTW) and evolve O2. Once the oceans saturated with the stuff, it leaked into the atmosphere. It could be called the first mass extinction, since the free living obligate anaerobes in the oceans were killed by the O2. Another consequence of the oxygenation event was that metal oxides, in particular iron oxides, were formed in the oceans; and being insoluble, precipitated onto the ocean floors. The rocks that formed from these possesses a characteristic texture of alternating red oxide interspersed with layers of ordinary sediments. This is the source of "banded iron formations" that constitute the massive and massively exploited ore deposits in Minnesota and Australia, I believe.
 
  • #33
Cyanobacteria is a phylum of bacteria. It's a good idea not to use the term "blue-green algae" at all.
 
  • #34
CapnGranite said:
Except that I think the evidence is increasing for the water-rich meteorite impacts not being necessary for the primary ocean formation. The volcanic activity suggests that deeper-seated water was brought to the surface by tectonic activity and the volcanism. The later bombardment by water-rich meteorites added to the water volume. I suppose there are two camps regarding the origin of the oceans, water-enstatite grains along with other mineral material, accreting to for the Earth and the group that invokes the bombardment as being the primary source of water. Since around 2011 and up to today, everybody I know and have spoken to favors the first model.
Well, up to a point, count me in as another "everybody".

My reservation is that I do not count bombardment as something that started only after accretion. As I see it, the early accretion lumps were part of the bombardments. However, that still leaves me supporting my original view (pre-1990s at least) that the post-accretion bombardment, including any residual items that still land about our ears today, are trivial tail-enders that couldn't really have played much of a role in enriching the planet with anything special, including organics and volatiles, except for a few rare, siderophilic elements such as iridium. The main difference is that in the last few billion years they might have undergone a loss of volatiles and some partitioning of isotopes etc.

Accordingly the bombardment as usually so described would not have been likely to have had much influence either on the formation of oceans or on the origin of life on Earth.

My $2000000-worth (to accommodate inflation since the Ordovician) :biggrin:
 
  • #35
Fervent Freyja said:
Bacteria.

My take on this ordeal: Prior to ocean formation the atmosphere had been mainly hydrogen, helium, methane, and ammonia. It is now believed that much of the water and rock had been locked into the crust, at the same time, during formation and that a small contribution was made by water-rich meteorite impacts. A lot of volcanic activity released water vapor into the atmosphere, along with carbon dioxide; which, then formed heavy clouds over the Earth that rained for a long time- eventually, forming the ocean. Water came first, not oxygen.
Bacteria is life-one of three kinds of life. This form of life might have done the job-or it might have been done by chemistry not involving life at all. Or maybe a little of both. The point is CO2 locked up in rocks was in the atmosphere early on and there is a lot of CO2 locked up in rocks.
 
  • #36
Fervent Freyja said:
I do think you are right. It may be more right to say that water was locked into the crust as material accreted and later impacts may have contributed some.

Still, this explanation doesn't satisfy me. Something is off. Looking at all the advancements we have made (look at what we can describe about the universe) and comparing it to how little we can explain about the formation of the early Earth makes me uncomfortable.
I wonder if anyone has considered buoyancy in these models? It seems to me water will tend to rise to the surface because the crust is much denser and will tend to sink in water. I know water fills holes in the crust but how deep down do conditions exist for holes to develop?
 
  • #37
jim meyer said:
Well let's not nitpick-I agree photosynthesis has added O2 to the atmosphere. My point is free oxygen has always been in the atmosphere at about 10E18kg or so. The fact that much more CO2 was in the early atmosphere(CO2 now in rocks)and dwarfs the other gases. This is not known and I just want you to do a calculation of how much CO2 rocks like calcite, dolomite and other rocks have absorbed from the early atmosphere. Not rocket science in any way.
Not much to ask I suppose, but some of your views are confusingly expressed, to put it diplomatically. Chemically and biologically speaking for example, CO2 is not regarded as free oxygen, and the point is not purely academic, as you will find out if you try inhaling some. I agree that the early Earth's atmosphere would have contained plenty of CO2 until the rocks cooled down to something like 200C. But that is not free O2, and its difference from free O2 would affect all sorts of things from physical atmospheric characteristics to the precipitation of huge quantities of silica from silicates. Photosynthesis of free O2 in large quantities was one of the great pollution events in the (pre)history of the planets where there had never before been more than traces of anything so violently destructive or toxic before. Not merely whole species, but whole ecological complexes were wiped out within a few million years, and probably repeatedly at that during the transition ages.

If that is nit-picking, make the most of it.

Incidentally, while you are at doing your calculations, you might have some fun calculating how much CO2 is dissolved in the ocean right now, compared to how much we have in our atmosphere, and working out how it got there and how long it has been there, and what is important about it.

The natural world is full of surprises.
 
  • #38
jim meyer said:
I wonder if anyone has considered buoyancy in these models? It seems to me water will tend to rise to the surface because the crust is much denser and will tend to sink in water. I know water fills holes in the crust but how deep down do conditions exist for holes to develop?
As it happens, yes, people do consider buoyancy, but in the early planet temperature was far more important. Such water as wasn't firmly bound tended to gasify dramatically, and even today volcanic clouds contain lots of steam apart from their dust. The first oceans probably rained out of volcanic clouds long before they formed any noticeable puddles.

As for holes in the crust, below the top few km they tend to get squoze shut pretty quickly for the simple reason that most rock is plastic under pressure and at temperatures that superheat steam.

Water is generally a very scarce component of our planet and you will find hardly any even in the deep crust, let alone in the mantle. Actually, I did read somewhere of recent evidence that there might be more water in special regions of the mantle I think it was, than in the current oceans, but that still is small beer (if you will excuse the expression) compared to the overall volume and mass of the mantle and crust. Any volcano tapping such a source however, could do a lot of raining, it seems. :biggrin:
 
  • #39
jim meyer said:
Bacteria is life-one of three kinds of life. This form of life might have done the job-or it might have been done by chemistry not involving life at all. Or maybe a little of both. The point is CO2 locked up in rocks was in the atmosphere early on and there is a lot of CO2 locked up in rocks.

Actually that is by no means the point. How many kinds of life bacteria are, is a matter of definition. A lot of folks like to think of them as two kinds, and some prefer more. To argue one way or another one needs to explain first which purposes your classification serves. None of us has done that just here and now, because it does not address the original question.

But photosynthetic bacteria that process CO2 generally dissolve it from the air or use it dissolved in water. In other words, much as plants do. To extract it from rock is not vanishingly rare, but generally is a specialist adaptation to particular ecologies. A bit of a curiosity if you like.
 
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  • #40
Jon Richfield said:
Not much to ask I suppose, but some of your views are confusingly expressed, to put it diplomatically. Chemically and biologically speaking for example, CO2 is not regarded as free oxygen, and the point is not purely academic, as you will find out if you try inhaling some. I agree that the early Earth's atmosphere would have contained plenty of CO2 until the rocks cooled down to something like 200C. But that is not free O2, and its difference from free O2 would affect all sorts of things from physical atmospheric characteristics to the precipitation of huge quantities of silica from silicates. Photosynthesis of free O2 in large quantities was one of the great pollution events in the (pre)history of the planets where there had never before been more than traces of anything so violently destructive or toxic before. Not merely whole species, but whole ecological complexes were wiped out within a few million years, and probably repeatedly at that during the transition ages.

If that is nit-picking, make the most of it.

Incidentally, while you are at doing your calculations, you might have some fun calculating how much CO2 is dissolved in the ocean right now, compared to how much we have in our atmosphere, and working out how it got there and how long it has been there, and what is important about it.

The natural world is full of surprises.
Well I didn't mean to say CO2 was free oxygen if that is what you mean. The CO2 molecule is mostly oxygen and photosynthesis or inorganic chemistry can free the oxygen therein. There is a lot more CO2 in the ocean than in the atmosphere. Still more than 90% of all the CO2 on our lovely planet is locked in rocks.
 
  • #42
CapnGranite said:
http://www.astrobio.net/news-exclusive/scientists-detect-evidence-oceans-worth-water-Earth's-mantle/
SCIENTISTS DETECT EVIDENCE OF ‘OCEANS WORTH’ OF WATER IN EARTH’S MANTLE

http://science.sciencemag.org/content/344/6189/1265
This is the original paper, from 2014, but is still locked
Thanks yes, that was the one, though I can't remember whether I read the original or a popular version. But the abstract is adequate for our need here for the moment.
Mind you, it is an observation that opens intriguing lines of speculation. But they are rather academic. I bet that when we get to the technological stage of development that permits us to dig so deep, we'll find that the water is too dilute and too salty to be worth extracting.
But then again, if we could get down there, just extracting the water would be an energetically profitable operation...
Enormously, explosively profitable...
Hmmm...
And think about the mineral impurities -- if we can find water so deep, maybe we could find iridium so shallow... :wideeyed:
$$$$$$$$$$$$$$$$!
:biggrin:
 
  • #43
jim meyer said:
Well I didn't mean to say CO2 was free oxygen if that is what you mean. The CO2 molecule is mostly oxygen and photosynthesis or inorganic chemistry can free the oxygen therein. There is a lot more CO2 in the ocean than in the atmosphere. Still more than 90% of all the CO2 on our lovely planet is locked in rocks.
 
  • #44
Mark Harder said:
No, there are bacteria, called anaerobes, that can live in the absence of O2. In fact, there are anaerobes, called obligate anaerobes, that cannot live in the presence of oxygen, i.e. it's a poison to them.

Oh, but if you remember, oxygen is poisonous to most lifeforms anyway, especially humans... :biggrin:

From what I recall O2 levels in the GI tract range from 2-8% and some obligate anaerobes make it a home!
 
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  • #45
I'm not sure that 90% of CO2 per se is "locked in rocks". Large amounts can be locked up in clathrates, but rocks don't typically lock up CO2. This paper shows the complexity of carbonate species in the Earth system:
http://advances.sciencemag.org/content/2/10/e1601278.full
The fate of carbon dioxide in water-rich fluids under extreme conditions

Another interesting paper is:
http://dge.stanford.edu/SCOPE/SCOPE_16/SCOPE_16_1.5.05_Siegenthaler_249-257.pdf
13C/12C Fractionation during CO2 Transfer from Air to Sea

and another:
http://www.columbia.edu/~vjd1/carbon.htm
Carbonate Rocks

1. Carbon dioxide is removed from the atmosphere by dissolving in water and forming carbonic acid

CO2 + H2O -> H2CO3 (carbonic acid)
2. Carbonic acid is used to weather rocks, yielding bicarbonate ions, other ions, and clays

H2CO3 + H2O + silicate minerals -> HCO3- + cations (Ca++, Fe++, Na+, etc.) + clays
3. Calcium carbonate is precipitated from calcium and bicarbonate ions in seawater by marine organisms like coral

Ca++ + 2HCO3- -> CaCO3 + CO2 + H2O
the carbon is now stored on the seafloor in layers of limestone

 
  • #46
https://deepcarbon.net/feature/study-suggests-earth%E2%80%99s-carbon-originated-planetary-smashup#.WAgu6pMrL-a
The challenge is to explain the origin of the volatile elements like carbon that remain outside the core in the mantle portion of our planet,”

https://deepcarbon.net/content/dco-march-2013-press-release#.WAgvnZMrL-Z
Carbon: Quest Underway to Discover its Quantity, Movements, Origin, and Forms in Deep Earth
A small fraction of Earth's carbon is in its atmosphere, seawater and top crusts. An estimated 90% or more is locked away or in motion deep underground — a hidden dimension of the planet as poorly understood as it is profoundly important to life on the surface.

So, it might be correct to say that 90% of carbon is tied up in various ways in the rocks, but not CO2
 
  • #47
CapnGranite said:
I'm not sure that 90% of CO2 per se is "locked in rocks". Large amounts can be locked up in clathrates, but rocks don't typically lock up CO2. This paper shows the complexity of carbonate species in the Earth system:
http://advances.sciencemag.org/content/2/10/e1601278.full
The fate of carbon dioxide in water-rich fluids under extreme conditions
Good material and much thanks for the URLs. I still haven't read much of the material because I am playing hookey as things are, but one comparatively small, but actually highly important, reservoir is CO2 insecurely "locked" into solution in the deep sea. It has accumulated in deep layers under pressure, not all of it from the atmosphere. There is more than enough to kill us all if it were suitably released. I draw everyone's attention to the history of lake Nyos (https://en.wikipedia.org/wiki/Lake_Nyos) and leave readers unfamiliar with the history and mechanisms, to wonder why it has not yet happened.

And furthermore, given that its escape is inevitable, work out when it can no longer be averted. :wink:

As for "locking in rocks" in other forms than as carbonates or at an even remoter stretch, as organic compounds or inorganic carbides, I'd be surprised if that were important in any practical way. I cannot think of any sort of rock that can retain molecular CO2 except for bubbles in glassy volcanic rocks or pumice, and that is a pretty insignificant fraction, and one that does not generally escape catastrophically except as volcanic explosions. Lots of fun and amazingly photogenic, but percentage-wise trivial.

Non-gaseous forms of carbon (as opposed to CO2) in the Earth are mostly carbonates and organic compounds in the upper crust, but in the lower crust and mantle, carbides and free carbon would dominate, and though I have no information on them, I would bet a few cases of beer that they dominate the planetary carbon reserves. After all, our surface and shallow supplies are mercifully tiny.
 

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