juju7 wrote:Cito di Pense wrote:juju7 wrote:Cito di Pense wrote:All this says is that if you detect oxygen in the atmosphere of an extrasolar planet, it's not necessarily diagnostic of green plants down below. The tiny amounts of molecular oxygen that can be produced by, e.g., photodissociation of CO2 (not to mention H2O) will rapidly react with other molecular gases in the atmosphere, such as CO, CH4, H2S or atomic species which are even more reactive. Should that not be sufficient to convince you that not much free molecular oxygen will result, if there are any rocks on the planetary surface containing iron, there's another reservoir for soaking up molecular oxygen. Thus the concentration of oxygen in any planetary atmosphere above a planet not harboring green plants is likely to remain very, very low. Here on earth, the evolution of photosynthesis was a catastrophe for anaerobic bacteria. Earth's oxygen (at biologically-significant levels) is the outcome of photosynthesis. I don't think anyone participating in this thread will doubt this.
I do. You have failed to show that oxygen levels will be very low, and you don't explain why there should be reducing conditions in an atmosphere.
How long did it take you to come up with that boner? It's looking like more than a year.
Oxygen is very reactive, reacting quickly with other atmospheric species to make oxidized compounds like water, carbon dioxide, carbon monoxide and nitrogen oxides. When there is not a continuous supply of molecular oxygen, its concentration in a reducing atmosphere (an atmosphere without a continuing supply of oxygen) will remain low. Learn some fucking chemistry, for fuck's sake.
You didn't read my post.
Repeat: Why should there be reducing conditions in an atmosphere?
The atmosphere of Venus, for instance contains no reducing gasses that can react with oxygen.
Learn some manners, mate.
Then I guess there should be lots of free oxygen in the atmosphere of Venus, right? Mate? What sorts of processes do you think hinder the accumulation of free oxygen in the present atmosphere of Venus? Could it be that CO2 is a stable compound relative to C + O2 or CO + O* or CO4* + C* (and so on) under conditions found in the Venerian atmosphere? You know what they say: If it happens, it must be possible, and that should answer your feeble inquiry into why oxygen concentration is low in the Venerian atmosphere, unless you'd refuse to consider something like C* (g) a reducing gas species, given stability relations you can easily evaluate for atomic carbon and molecular oxygen and carbon dioxide at T,P(Venus atmosphere).
No one's explaining to you why there
should be reducing conditions in an atmosphere because that wasn't the question. Who says there
should be reducing conditions in an atmosphere? What's been said is that if reducing conditions exist, molecular oxygen is short-lived.
Specify a gas phase inorganic catalysis for generating molecular oxygen from CO2 at some temperature and pressure, write a dissertation on how this can happen without application of considerable engineering skill, and there will be a faculty position waiting for you at some prestigious university. Otherwise, use green plants.