There's not much left because it mostly boils off due to low pressure, but in dark crevasses it's likely to stay cold enough to remain condensed. It's been measured spectroscopically.
There's not much left because it mostly boils off due to low pressure, but in dark crevasses it's likely to stay cold enough to remain condensed. It's been measured spectroscopically.
The discovery of photosynthesis caused the "great oxygenation event" which pumped oxygen into the atmosphere. Oxygen reacts with atmospheric hydrogen to form water. Without the oxygen, the very light hydrogen molecules would float to the top of the atmosphere and are easily blown away by solar winds, which is what happened on Mars. But with high oxygen concentrations on Eath, hydrogen molecules react to form heavier water molecules before they have a chance to be blown away, and thus hydrogen and water are retained.
I read about this in the book "Oxygen" by Nick Lane.
His point in this new article is that instead of one big "oxygenation event" there may have been multiple. But he sticks to his story that the creation of an ozone layer by photosynthesis was the key step in saving the oceans. He argues both Mars and Earth had oceans originally (confirmed by Mars Satellite observations), which were gradually diminished by a process in which ultraviolet light splits atmospheric water, minerals on the surface absorbed the oxygen (rusting, making Mars red) leaving the hygrogen to blow away. But life on earth pumped extra oxygen into the atmosphere, faster than minerals could aborb it, creating the reactive ozone layer which prevented hydrogen from blowing away, thus saving the oceans from their fate on Mars.
[1] nick-lane.net/wp-content/uploads/2016/12/Oxygen-and-life.pdf
gravity and magnetic field? if it were hydrogen or helium it would be stripped off by solar wind (storms) like everywhere else, but water is quite heavy due to the oxygen.
also 'everywhere else' means practically mercur, mars and asteroids (moon). no idea about venus. ice giants keeps their water also due to gravity and far apart on pluto it's frozen like rock.
You forgot freeze.
I can't intelligently contribute to the overall discussion here, but I know one of the most interesting things about the currently understood timeline is the apparent lack of eons between the earliest conditions conducive to life after its initial cooling and the earliest evidence of life. Don't quote me on exact numbers, but within margins of error, as I understand it, it's like in the range of millions of years, not billions (which has all sorts of interesting implications for both the Fermi paradox and religious thinkers) Though, as far as I know, you'd still be correct on the distance to photosynthesis.
Or not; the “land theory” (that it began in shallow, possibly volcanic, terrestrial pools”) and “sea theory” (that it began in oceans, possibly at hydrothermal vents) have been competing theories forever, essentially.
Hydrogen comes from primordial nucleosynthesis [1] and makes up most of the interstellar medium [2]. Oxygen is produced when neutron stars collide and stars explode [3] as well as when some stars burn [4]. These freely combined in the gas disk from which our solar system formed, condensing into planets, moons, comets and other things [5].
[1] https://en.m.wikipedia.org/wiki/Big_Bang_nucleosynthesis
[2] http://casswww.ucsd.edu/archive/public/tutorial/ISM.html
[3] https://www.chemistryworld.com/news/heavy-elements-forged-by...
Also, we seem to have a lot of water. It's really all from comets, a little here, a little there?
So at the time of the formation of the solar system, the whole area was a big gaseous cloud of supernova debris with lots of ice. The ignition of the sun started the frost line, and pushed volatiles out of the inner solar system. However some had already been trapped in the formation of the planets, and rose to the surface as they cooled. That's where Earth's ocean came from, and we know Mars and Venus had oceans too. Presumably also Mercury, although I'm sure that was short-lived.
So yes, it's all from cometary material. But then ALL of the Earth is from cometary material, and the oceans only make up a small amount of the Earth's total mass.
We’re not sure from where Earth’s water came [1]. Some evidence suggests the Earth was born with all its water, some that most came from comets.
[1] https://en.m.wikipedia.org/wiki/Origin_of_water_on_Earth
The water on Earth may seem to be a lot to us on the surface but it is only about 0.02% by mass [1].
https://www.universetoday.com/65588/what-percent-of-earth-is...
Oxygen is pretty common and hydrogen is everywhere, so water (as ice) is not scarce in the universe. The only place where water is uncommon is near a star, like us, where the water boils off into space unless a planet has enough gravity to hold it in.
I think the concept you're thinking of is free energy, which determines the final destination of a process. The equation relating these things is (change in free energy) = (change in energy) - temperature × (change in entropy). Entropy only becomes the dominant component when temperature is high. And, as expected, water molecules dissociate at high temperature.
In any case: dH=TdS + Vdp note dp is small in space but V can be large and dS is the change in entropy.
...and enthalpy of ideal (interstellar H & O) gases does not depend on pressure, unlike entropy and Gibbs energy. If you really just mean free energy U, then they are basically the same thing in open space (but not in a plasma), a distinction without difference.
For further pedantics I recommend Wikipedia, since I doubt we are helping anyone else.
So in a stellar accretion disc, much of the water will end up inside the new star, and dissociate, but quite a lot of it will gather in the planets, moons, and comets. Europa, for example, has about 2 or 3 Earth-oceans worth of water. Uranus and Neptune likely have solid cores composed mainly of ices that include water ice.
Water is fairly abundant in the universe. As are alcohols.
-- Ian Banks