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  2. Deuterium - Wikipedia

    en.wikipedia.org/wiki/Deuterium

    This is the ratio found in the gas giant planets, such as Jupiter. The analysis of deuterium–protium ratios (2 H 1 HR) in comets found results very similar to the mean ratio in Earth's oceans (156 atoms of deuterium per 10 6 hydrogen atoms). This reinforces theories that much of Earth's ocean water is of cometary origin.

  3. Heavy water - Wikipedia

    en.wikipedia.org/wiki/Heavy_water

    Since one in about every 6,400 hydrogen atoms is deuterium, a 50-kilogram (110 lb) human containing 32 kilograms (71 lb) of body water would normally contain enough deuterium (about 1.1 grams or 0.039 ounces) to make 5.5 grams (0.19 oz) of pure heavy water, so roughly this dose is required to double the amount of deuterium in the body.

  4. Origin of water on Earth - Wikipedia

    en.wikipedia.org/wiki/Origin_of_water_on_Earth

    The deuterium to hydrogen ratio for ocean water on Earth is known very precisely to be (1.5576 ± 0.0005) × 10 −4. [35] This value represents a mixture of all of the sources that contributed to Earth's reservoirs, and is used to identify the source or sources of Earth's water.

  5. Semiheavy water - Wikipedia

    en.wikipedia.org/wiki/Semiheavy_water

    On Earth, semiheavy water occurs naturally in normal water at a proportion of about 1 molecule in 3,200; because 1 in 6,400 hydrogen atoms in water is deuterium, which is 1 part in 3,200 by weight. HDO may be separated from normal water by distillation or electrolysis , or by various chemical exchange processes, all of which exploit a kinetic ...

  6. Global meteoric water line - Wikipedia

    en.wikipedia.org/wiki/Global_meteoric_water_line

    The Global Meteoric Water Line (GMWL) describes the global annual average relationship between hydrogen and oxygen isotope (oxygen-18 [18 O] and deuterium [2 H]) ratios in natural meteoric waters. The GMWL was first developed in 1961 by Harmon Craig, and has subsequently been widely used to track water masses in environmental geochemistry and ...

  7. Water distribution on Earth - Wikipedia

    en.wikipedia.org/wiki/Water_distribution_on_Earth

    Most water in Earth's atmosphere and crust comes from saline seawater, while fresh water accounts for nearly 1% of the total. The vast bulk of the water on Earth is saline or salt water, with an average salinity of 35‰ (or 3.5%, roughly equivalent to 34 grams of salts in 1 kg of seawater), though this varies slightly according to the amount of runoff received from surrounding land.

  8. Hydrogen isotope biogeochemistry - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_isotope...

    The deuterium used in the experiment was a generous gift of heavy water from UC Berkeley physicist Gilbert N. Lewis. [4] Bombarding deuterium produced two previously undetected isotopes, helium-3 (3 He) and 3 H. Rutherford and his colleagues successfully created 3 H, but incorrectly assumed that 3 He was the radioactive

  9. Water on terrestrial planets of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Water_on_terrestrial...

    The current Venusian atmosphere has only ~200 mg/kg H 2 O(g) in its atmosphere and the pressure and temperature regime makes water unstable on its surface. Nevertheless, assuming that early Venus's H 2 O had a ratio between deuterium (heavy hydrogen, 2H) and hydrogen (1H) similar to Earth's Vienna Standard Mean Ocean Water of 1.6×10 −4, [7] the current D/H ratio in the Venusian atmosphere ...