Halogens in the context of "Volatile (astrogeology)"

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⭐ Core Definition: Halogens

The halogens (/ˈhæləən, ˈh-, -l-, -ˌɛn/) are a group in the periodic table consisting of six chemically related elements: fluorine (F), chlorine (Cl), bromine (Br), iodine (I), and the radioactive elements astatine (At) and tennessine (Ts), though some authors would exclude tennessine as its chemistry is unknown and is theoretically expected to be more like that of gallium. In the modern IUPAC nomenclature, this group is known as group 17.

The word "halogen" means "salt former" or "salt maker". When halogens react with metals, they produce a wide range of salts, including calcium fluoride, sodium chloride (common table salt), silver bromide, and potassium iodide.

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👉 Halogens in the context of Volatile (astrogeology)

Volatiles are the group of chemical elements and chemical compounds that can be readily vaporized. In contrast with volatiles, elements and compounds that are not readily vaporized are known as refractory substances.

On planet Earth, the term 'volatiles' often refers to the volatile components of magma. In astrogeology volatiles are investigated in the crust or atmosphere of a planet or moon. Volatiles include hydrogen, nitrogen, oxygen, water, ammonia, methane, carbon dioxide, nitrogen dioxide, sulfur dioxide, hydrogen sulfide, phosphine, halogens, noble gases and others.

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