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Mercury (element)

Chemical element with atomic number 80 (Hg)

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Element mercury (Hg), liquid form.
Bionerd · CC BY 3.0

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Mercury occurs in deposits throughout the world mostly as cinnabar (mercuric sulfide). The red pigment vermilion is obtained by grinding natural cinnabar or synthetic mercuric sulfide. Exposure to mercury and mercury-containing organic compounds is toxic to the nervous system, immune system and kidneys of humans and other animals; mercury poisoning can result from exposure to water-soluble forms of mercury (such as mercuric chloride or methylmercury) either directly or through mechanisms of biomagnification.

Mercury is used in thermometers, barometers, manometers, sphygmomanometers, float valves, mercury switches, mercury relays, fluorescent lamps and other devices, but concerns about the element's toxicity have led to a reduction in the amount of mercury used in these instruments, or manufacturers not using it altogether. It remains in use in scientific research applications and in amalgam for dental restoration in some locales. It is also still used in fluorescent lighting, although the quantity of mercury used is now smaller. Electricity passed through mercury vapor in a fluorescent lamp produces short-wave ultraviolet light, which then causes the phosphor in the tube to fluoresce, making visible light.

Properties

Physical properties

Mercury is a heavy, silvery-white metal. It is the only metallic element that is known to be liquid at standard temperature and pressure; the only other element that is liquid under these conditions is bromine, one of the halogens, though metals such as caesium, gallium, and rubidium melt just above room temperature. Compared to other metals, mercury is a poor conductor of heat, but a fair conductor of electricity.

Mercury has a melting point of −38.83 °C (−37.89 °F; 234.32 K) and a boiling point of 356.73 °C (674.11 °F; 629.88 K) both the lowest of any stable metal, resulting in the lowest stable liquid-state range of any metal under standard conditions. This effect is due to lanthanide contraction and relativistic contraction reducing the orbit radius of the outermost electrons, and thus weakening the metallic bonding in mercury. Upon freezing, the volume of mercury decreases by 3.59% and its density changes from 13.69 g/cm3 when liquid to 14.184 g/cm3 when solid. The coefficient of volume expansion is 181.59 × 10−6 at 0 °C, 181.71 × 10−6 at 20 °C and 182.50 × 10−6 at 100 °C (per °C). Solid mercury is malleable and ductile, and can be cut with a knife.

When expanded by heating near its critical point (around 1,750 K (1,480 °C; 2,690 °F) and 1,720 bars (172 MPa)), mercury exhibits a metal-nonmetal transition associated with sharp changes in its electronic conductivity and optical properties.

Mercury was the first known superconductor, discovered in 1911 by Heike Kamerlingh Onnes by cooling of mercury below 4 K (−269.15 °C; −452.47 °F) shortly after the discovery and production of liquid helium. Its superconductive properties were later determined to be unusual compared to other later-discovered superconductors, such as the more popular niobium alloys.

At room temperature (20 °C (293 K; 68 °F)), liquid mercury solidifies into a simple rhombohedral structure at approximately 1.2 gigapascals (12,000 bar) of pressure. On further compression, mercury undergoes several structural phase transitions into at least four distinct solid allotropes as compression increases, where the δ-phase with an hexagonal-close-packed (hcp) structure is stable above 36 gigapascals (360,000 bar) until at least 200 gigapascals (2,000,000 bar). The melting curve at high-pressure increases steeply on initial compression, but exhibits a pronounced flattening and a potential local maximum at around 9 gigapascals (90,000 bar). At 1 standard atmosphere (1.0 bar; 0.10 MPa)), liquid mercury exhibits an anomalously low first-shell coordination number, with each Hg atom having around 6 to 10 nearest neighbours, in contrast to simple metallic liquids in which atoms are densely-packed with 12 nearest neighbours. At simultaneous high-pressure and temperature conditions, the atomic arrangement in liquid mercury progresses towards a simple densely packed liquid structure. However, even at very high pressures (up to around 10 gigapascals (100,000 bar)), liquid mercury retains more many-body clusters than expected for a simple hard-sphere liquid.

Chemical properties

Mercury is somewhat more reactive than the noble metals gold and platinum that are close to it in the periodic table, but it is more stable than other the group 12 metals, zinc and cadmium. It reacts with oxidizing acids such as concentrated sulfuric acid and nitric acid or aqua regia to give mercury(II) sulfate, mercury(II) nitrate, and mercury(II) chloride, respectively. Like silver, mercury reacts with atmospheric hydrogen sulfide. Mercury reacts with solid sulfur flakes, which are used in mercury spill kits to absorb mercury (spill kits also use activated carbon and powdered zinc).

Amalgams

Mercury dissolves many metals such as gold and silver to form amalgams. Iron is an exception, and iron flasks have traditionally been used to transport the material. Several other first row transition metals (with the exception of manganese, copper and zinc) are also resistant in forming amalgams. Other elements that do not readily form amalgams with mercury include platinum. Sodium amalgam is a common reducing agent in organic synthesis, and is also used in high-pressure sodium lamps.

Mercury readily combines with aluminium to form a mercury-aluminium amalgam when the two pure metals come into contact. Since the amalgam destroys the aluminium oxide layer which protects metallic aluminium from oxidizing in-depth (as in iron rusting), even small amounts of mercury can seriously corrode aluminium. For this reason, mercury is not allowed aboard an aircraft under most circumstances because of the risk of it forming an amalgam with exposed aluminium parts in the aircraft.

Mercury embrittlement is the most common type of liquid metal embrittlement, as mercury is a natural component of some hydrocarbon reservoirs and will come into contact with petroleum processing equipment under normal conditions.

Isotopes

There are seven stable isotopes of mercury, with 202Hg being the most abundant (29.86%). The longest-lived radioisotopes are 194Hg with a half-life of 444 years, and 203Hg with a half-life of 46.612 days. Most of the remaining radioisotopes have half-lives that are less than a day. 206Hg occurs naturally in tiny traces as an intermediate decay product of 238U. 199Hg and 201Hg are the most often studied NMR-active nuclei, having spins of 1⁄2 and 3⁄2 respectively.

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