When you think about the zork fittings,I still don't know what the shells are for. But the tongs are starting to make sense.
it all comes together.
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When you think about the zork fittings,I still don't know what the shells are for. But the tongs are starting to make sense.
An opinion is just an onion with pi.
(I'm disappointed that you ignored my bogus math.)
Is there deuterium on Mars?Why would you believe that? It may have a slightly higher amount of deuterium than our water does, but I do not see how it could possibly be D2O.
I'd prefer to leave myself and let the MAGAs have this rock.I would hope for a mass exodus of a MAGAnificent group of people and this country would finally be great again.
I think they have all the rocks they need and have space for.I'd prefer to leave myself and let the MAGAs have this rock.
Thank you for supporting my claim and refuting yours. Even at six times our amount of deuterium water would be almost pure H1 or protonium if you prefer. Even with the highest value by that one measurement it would still be less than one hydrogen atom out of 1,000 being deuterium.Is there deuterium on Mars?
An approximately six-fold deuterium-to-hydrogen (D/H or 2H/1H) enrichment in Martian water vapor relative to standard mean ocean water (SMOW, D/H = 1.56 × 10 − 4 ) was first detected spectroscopically (Owen et al., 1988) and has since been confirmed by in-situ measurements of Mars's atmosphere (Webster et al., 2013).Oct 1, 2022
Mars has very little atmosphere. So like water all over the universe, the hydrogen is always open to evolving with direct sun em. (Light)Thank you for supporting my claim and refuting yours. Even at six times our amount of deuterium water would be almost pure H1 or protonium if you prefer. Even with the highest value by that one measurement it would still be less than one hydrogen atom out of 1,000 being deuterium.
That does not change the hydrogen nucleus. That takes nuclear physics. You won't see that happening unless you are very deep down inside the Sun.Mars has very little atmosphere. So like water all over the universe, the hydrogen is always open to evolving with direct sun em. (Light)
I was not trying to see it. And the suns solar wind is conveying the elements from the sun's nuclear works. The sun (stars) do the work and the physics are describing the model, not making it happen.That does not change the hydrogen nucleus. That takes nuclear physics. You won't see that happening unless you are very deep down inside the Sun.
You described the "evolution" of hydrogen as if sunlight could change the nucleus. As if hydrogen could capture a free neutron or helium could decay into 2 deuterium nuclei under sunlight.I was not trying to see it. And the suns solar wind is conveying the elements from the sun's nuclear works. The sun (stars) do the work and the physics are describing the model, not making it happen.
You're kind of cute.
Mars has very little atmosphere. So like water all over the universe, the hydrogen is always open to evolving with direct sun em. (Light)
No, everyone in the world looks up and sings "America! **** Yeah!"95% of the world population would not be happy
""You described the "evolution" of hydrogen as if sunlight could change the nucleus. As if hydrogen could capture a free neutron or helium could decay into 2 deuterium nuclei under sunlight.
And that would be a trifling amount..""
Abstract
A measurement of the intensities of cosmic-ray-produced deuterium and tritium in the earth's atmosphere has been made using a dE/dx and E detector flown aboard two high-altitude balloon flights launched from Fort Churchill, Manitoba, in June 1965."""
That's over half a century old.
And not what you stated above.""
Abstract
A measurement of the intensities of cosmic-ray-produced deuterium and tritium in the earth's atmosphere has been made using a dE/dx and E detector flown aboard two high-altitude balloon flights launched from Fort Churchill, Manitoba, in June 1965."""
That's over half a century old.
Cosmic rays come from stars. Including the sun.And not what you stated above.
1. Those are cosmic rays, not sunlight.
2. It doesn't describe the formation of deuterium from hydrogen.
See also: Cosmic-ray production of deuterium, He3, lithium, beryllium, and boron in the Galaxy - Astrophysics and Space Science
Here is something I predicted 20 years ago and has recently been verified by science.You started off doing fine, but then you began to spout nonsense. You need to find sources that say the water cycle has anything at all to do with our magnetic field. In fact from that point on you just yammered your own pseudoscience.
So it’s not D2O then. The 6-fold higher, but still tiny, proportion of deuterium compared to that on Earth is apparently due to a greater degree of fractionation by the escape into space of the lighter isotope.Is there deuterium on Mars?
An approximately six-fold deuterium-to-hydrogen (D/H or 2H/1H) enrichment in Martian water vapor relative to standard mean ocean water (SMOW, D/H = 1.56 × 10 − 4 ) was first detected spectroscopically (Owen et al., 1988) and has since been confirmed by in-situ measurements of Mars's atmosphere (Webster et al., 2013).Oct 1, 2022
Okay, almost none of the water on Mars is going to be D2O. I am leaving the error bars off of this to keep it simple and rounding up, which is in your favor. One out of a thousand hydrogen atoms will be deuterium on Mars. That means that one out of a thousand water molecules on Mars will be PDO, or protonium deuterium oxide. It is only 5% more massive than H2O. The difference in heat of evaporation will also be about half way in between the two figures that you gave. Only one out of a million water molecules will be D20.The earth's conditions have liquid water and clouds and a strong sun for evaporation of water in bulk. The water on Mars is more solid water; ice, with more sublimation. Heavy water with deuterium is 10% denser than regular water, has a heat of vaporization of 41.521 kJ/mole, while the heat of vaporization of regular water is 40.657 KJ/mole. The regular water will evaporate slightly leaving behind an enrichment of D2O, on the cold Mars ice surface and atmosphere.