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Nova Centauri 2013 is the first in which evidence of lithium has been found. [13] Lithium is also found in brown dwarf substellar objects and certain anomalous metal-poor stars. Because lithium is present in cooler, less massive brown dwarfs, but is destroyed in hotter red dwarf stars, its presence in the stars' spectra can be used in the ...
At 20 mg lithium per kg of Earth's crust, [53] lithium is the 31st most abundant element. [54] According to the Handbook of Lithium and Natural Calcium, "Lithium is a comparatively rare element, although it is found in many rocks and some brines, but always in very low concentrations. There are a fairly large number of both lithium mineral and ...
Lithium can be removed from solution by formation of secondary minerals like clays, oxides, or zeolites. [1] Rivers eventually feed into the ocean, providing approximately 50% of marine inputs. [2] The remainder of lithium inputs come from hydrothermal venting at mid-ocean ridges, where lithium is released from the mantle. [1]
A stimulus to the development of the theory of nucleosynthesis was the discovery of variations in the abundances of elements found in the universe. The need for a physical description was already inspired by the relative abundances of the chemical elements in the solar system.
One must multiply by 3 (the molecular mass of helium-3) and divide by 29 (the mean molecular mass of the atmosphere), resulting in 3,828 tonnes (3,768 long tons; 4,220 short tons) of helium-3 in the earth's atmosphere.) 3 He is produced on Earth from three sources: lithium spallation, cosmic rays, and beta decay of tritium (3 H).
The overwhelming majority of rare-earth elements, tantalum, and lithium are found within pegmatite. Ore genesis theories for these ores are wide and varied, but most involve metamorphism and igneous activity. [10] Lithium is present as spodumene or lepidolite within pegmatite. Carbonatite intrusions are an important source of these elements ...
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The process results in the light elements beryllium, boron, and lithium in the cosmos at much greater abundances than they are found within solar atmospheres. The quantities of the light elements 1 H and 4 He produced by spallation are negligible relative to their primordial abundance.