Editing Goldschmidt classification (section)

==Lithophile elements==
Lithophile elements ({{ety|grc|''{{lang|grc|λῐ́θος}}'' ({{Transliteration|grc|líthos}})|stone||''{{lang|grc|φίλος}}'' ({{Transliteration|grc|phílos}})|dear, beloved}}) are those that remain on or close to the surface because they combine readily with oxygen, forming compounds that did not sink into the [[Earth's core]]. The lithophile elements include [[Aluminium|Al]], [[Boron|B]], [[Barium|Ba]], [[Beryllium|Be]], [[Bromine|Br]], [[Calcium|Ca]], [[Chlorine|Cl]], [[Chromium|Cr]], [[Caesium|Cs]], [[Fluorine|F]], [[Iodine|I]], [[Hafnium|Hf]], [[Potassium|K]], [[Lithium|Li]], [[Magnesium|Mg]], [[Sodium|Na]], [[Niobium|Nb]], [[Oxygen|O]], [[Phosphorus|P]], [[Rubidium|Rb]], [[Scandium|Sc]], [[Silicon|Si]], [[Strontium|Sr]], [[Tantalum|Ta]], [[Thorium|Th]], [[Titanium|Ti]], [[Uranium|U]], [[Vanadium|V]], [[Yttrium|Y]], [[Zirconium|Zr]], [[Tungsten|W]] and the [[lanthanide]]s or rare earth elements (REE).

Lithophile elements mainly consist of the highly reactive metals of the [[s-block|s-]] and [[f-block]]s. They also include a small number of reactive nonmetals, and the more reactive metals of the [[d-block]] such as [[titanium]], [[zirconium]] and [[vanadium]].

Most lithophile elements form very stable [[ion]]s with an [[electron configuration]] of a noble gas (sometimes with additional f-electrons). The few that do not, such as silicon, phosphorus and boron, form strong [[covalent bond]]s with oxygen, often involving [[pi bonding]]. Their strong affinity for oxygen causes lithophile elements to associate very strongly with [[silica]], forming relatively low-density minerals that thus rose towards the crust during [[planetary differentiation]]. The more soluble minerals formed by the [[alkali metal]]s tend to concentrate in [[seawater]] or [[Aridity|arid regions]] where they can crystallise. The less soluble lithophile elements are concentrated on ancient [[Shield (geology)|continental shields]] where soluble minerals have been weathered.

Because of their strong affinity for oxygen, most lithophile elements are enriched in the Earth's crust relative to their abundance in the [[Solar System]]. The most reactive s- and f-block metals, which form either saline or [[metallic hydrides]], are known to be extraordinarily enriched on Earth as a whole relative to their solar abundances. This is because during the earliest stages of the [[Earth's formation]], the abundance of stable forms of each element was determined by how readily it forms volatile hydrides; these volatiles then could "escape" the proto-Earth, leaving behind those elements unreactive with hydrogen. Under these conditions, the s- and f-block metals were strongly enriched during the formation of the Earth. The most enriched elements are [[rubidium]], [[strontium]] and [[barium]], which between them account for over 50 [[percent by mass]] of all [[elements heavier than iron]] in the Earth's crust.

The nonmetallic lithophiles{{snd}}[[phosphorus]] and the [[halogen]]s{{snd}}exist on Earth as ionic [[salts]] with s-block metals in [[pegmatite]]s and seawater. With the exception of [[fluorine]], whose [[hydride]] forms [[hydrogen bond]]s and is therefore of relatively low volatility, these elements have had their concentrations on Earth significantly reduced through escape of volatile hydrides during the Earth's formation. Although they are present in the Earth's crust in concentrations quite close to their solar abundances, phosphorus and the heavier halogens are probably significantly depleted ''on Earth as a whole'' relative to their solar abundances.

Several transition metals, including [[chromium]], [[molybdenum]], [[iron]] and [[manganese]], show ''both'' lithophile ''and'' siderophile characteristics and can be found in both these two layers. Although these metals form strong bonds with oxygen and are never found in the Earth's crust in the free state, metallic forms of these elements are thought very likely to exist in the core of the earth as relics from when the atmosphere did not contain oxygen. Like the "pure" siderophiles, these elements (except iron) are considerably depleted in the crust relative to their solar abundances.

Owing to their strong affinity for oxygen, lithophile metals, although they form the great bulk of the metallic elements in Earth's crust, were never available as free metals before the development of [[electrolysis]]. With this development, many lithophile metals are of considerable value as structural metals ([[magnesium]], [[aluminium]], [[titanium]], [[vanadium]]) or as [[reducing agents]] ([[sodium]], [[magnesium]], [[calcium]]).

The non-metals phosphorus and the halogens were also not known to early chemists, though production of these elements is less difficult than of metallic lithophiles since electrolysis is required only with fluorine. Elemental [[chlorine]] is particularly important as an [[oxidizing agent]]{{snd}}usually being made by electrolysis of [[sodium chloride]].