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Ammonia
Ammonia
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Ammonia
Stereo structural formula of the ammonia molecule
Stereo structural formula of the ammonia molecule
Ball-and-stick model of the ammonia molecule
Ball-and-stick model of the ammonia molecule
Space-filling model of the ammonia molecule
Space-filling model of the ammonia molecule
Names
IUPAC name
Ammonia[1]
Systematic IUPAC name
Azane
Other names
  • Hydrogen nitride
  • R-717
  • R717 (refrigerant)
  • Amidogen
  • Hydrogen amine
  • Nitrogen hydride
Identifiers
3D model (JSmol)
3587154
ChEBI
ChEMBL
ChemSpider
ECHA InfoCard 100.028.760 Edit this at Wikidata
EC Number
  • 231-635-3
79
KEGG
MeSH Ammonia
RTECS number
  • BO0875000
UNII
UN number 1005
  • InChI=1S/H3N/h1H3 checkY
    Key: QGZKDVFQNNGYKY-UHFFFAOYSA-N checkY
  • InChI=1/H3N/h1H3
    Key: QGZKDVFQNNGYKY-UHFFFAOYAF
  • N
Properties
NH3
Molar mass 17.031 g·mol−1
Appearance Colourless gas
Odor Strong pungent odour
Density
  • 0.86 kg/m3 (1.013 bar at boiling point)
  • 0.769 kg/m3 (STP)[2]
  • 0.73 kg/m3 (1.013 bar at 15 °C)
  • 0.6819 g/cm3 at −33.3 °C (liquid)[3] See also Ammonia (data page)
  • 0.817 g/cm3 at −80 °C (transparent solid)[4]
Melting point −77.73 °C (−107.91 °F; 195.42 K) (Triple point at 6.060 kPa, 195.4 K)
Boiling point −33.34 °C (−28.01 °F; 239.81 K)
Critical point (T, P) 132.4 °C (405.5 K), 111.3 atm (11,280 kPa)
  • 530g/l(20 °C)
  • 320g/l(25 °C)[5]
Solubility soluble in chloroform, ether, ethanol, methanol
Vapor pressure 857.3 kPa
Acidity (pKa) 32.5 (−33 °C),[6] 9.24 (of ammonium)
Basicity (pKb) 4.75
Conjugate acid Ammonium
Conjugate base Amide
−18.0×10−6 cm3/mol
1.3327
Viscosity
  • 10.07 µPa·s (25 °C)[7]
  • 0.276 mPa·s (−40 °C)
Structure
C3v
Trigonal pyramid
1.42 D
Thermochemistry
193 J/(mol·K)[8]
−46 kJ/mol[8]
Hazards
GHS labelling:[11]
GHS05: Corrosive GHS06: Toxic GHS09: Environmental hazard
Danger
H314, H331, H410
P260, P273, P280, P303+P361+P353, P304+P340+P311, P305+P351+P338+P310
NFPA 704 (fire diamond)
651 °C (1,204 °F; 924 K)
Explosive limits 15.0–33.6%
Lethal dose or concentration (LD, LC):
350 mg/kg (rat, oral)[9]
  • 40,300 ppm (rat, 10 min)
  • 28,595 ppm (rat, 20 min)
  • 20,300 ppm (rat, 40 min)
  • 11,590 ppm (rat, 1 hr)
  • 7338 ppm (rat, 1 hr)
  • 4837 ppm (mouse, 1 hr)
  • 9859 ppm (rabbit, 1 hr)
  • 9859 ppm (cat, 1 hr)
  • 2000 ppm (rat, 4 hr)
  • 4230 ppm (mouse, 1 hr)[10]
  • 5000 ppm (mammal, 5 min)
  • 5000 ppm (human, 5 min)[10]
NIOSH (US health exposure limits):[12]
PEL (Permissible)
50 ppm (25 ppm ACGIH-TLV; 35 ppm STEL)
REL (Recommended)
TWA 25 ppm (18 mg/m3) ST 35 ppm (27 mg/m3)
IDLH (Immediate danger)
300 ppm
Safety data sheet (SDS) ICSC 0414 (anhydrous)
Related compounds
Related nitrogen hydrides
Related compounds
Supplementary data page
Ammonia (data page)
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
checkY verify (what is checkY☒N ?)

Ammonia is an inorganic chemical compound of nitrogen and hydrogen with the formula NH3. A stable binary hydride and the simplest pnictogen hydride, ammonia is a colourless gas with a distinctive pungent smell.[13] It is widely used in fertilizers, refrigerants, explosives, cleaning agents, and is a precursor for numerous chemicals.[13] Biologically, it is a common nitrogenous waste, and it contributes significantly to the nutritional needs of terrestrial organisms by serving as a precursor to fertilisers.[14] Around 70% of ammonia produced industrially is used to make fertilisers[15] in various forms and composition, such as urea and diammonium phosphate. Ammonia in pure form is also applied directly into the soil.

Ammonia, either directly or indirectly, is also a building block for the synthesis of many chemicals. In many countries, it is classified as an extremely hazardous substance.[16] Ammonia is toxic, causing damage to cells and tissues. For this reason it is excreted by most animals in the urine, in the form of dissolved urea.

Ammonia is produced biologically in a process called nitrogen fixation, but even more is generated industrially by the Haber process. The process helped revolutionize agriculture by providing cheap fertilizers. The global industrial production of ammonia in 2021 was 235 million tonnes.[17][18] Industrial ammonia is transported by road in tankers, by rail in tank wagons, by sea in gas carriers, or in cylinders.[19] Ammonia occurs in nature and has been detected in the interstellar medium.

Ammonia boils at −33.34 °C (−28.012 °F) at a pressure of one atmosphere, but the liquid can often be handled in the laboratory without external cooling. Household ammonia or ammonium hydroxide is a solution of ammonia in water.

Etymology

[edit]

The name ammonia is derived from the name of the Egyptian deity Amun (Ammon in Greek) since priests and travelers of those temples would burn soils rich in ammonium chloride, which came from animal dung and urine.[13] Pliny, in Book XXXI of his Natural History, refers to a salt named hammoniacum, so called because of the proximity of its source to the Temple of Jupiter Amun (Greek Ἄμμων Ammon) in the Roman province of Cyrenaica.[20] However, the description Pliny gives of the salt does not conform to the properties of ammonium chloride. According to Herbert Hoover's commentary in his English translation of Georgius Agricola's De re metallica, it is likely to have been common sea salt.[21] In any case, that salt ultimately gave ammonia and ammonium compounds their name.

Natural occurrence (abiological)

[edit]

Traces of ammonia/ammonium are found in rainwater. Ammonium chloride (sal ammoniac), and ammonium sulfate are found in volcanic districts. Crystals of ammonium bicarbonate have been found in Patagonia guano.[22]

Ammonia is found throughout the Solar System on Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto, among other places: on smaller, icy bodies such as Pluto, ammonia can act as a geologically important antifreeze, as a mixture of water and ammonia can have a melting point as low as −100 °C (−148 °F; 173 K) if the ammonia concentration is high enough and thus allow such bodies to retain internal oceans and active geology at a far lower temperature than would be possible with water alone.[23][24] Substances containing ammonia, or those that are similar to it, are called ammoniacal.[25]

Properties

[edit]
Liquid ammonia
Liquid NH3
Solid ammonia
Solid NH3
Two visible states of NH3

Ammonia is a colourless gas with a characteristically pungent smell. It is lighter than air, its density being 0.589 times that of air. It is easily liquefied due to the strong hydrogen bonding between molecules. Gaseous ammonia turns to a colourless liquid, which boils at −33.1 °C (−27.58 °F), and freezes to colourless crystals[22] at −77.7 °C (−107.86 °F). Little data is available at very high temperatures and pressures, but the liquid-vapor critical point occurs at 405 K and 11.35 MPa.[26]

Solid

[edit]

The crystal symmetry is cubic, Pearson symbol cP16, space group P213 No.198, lattice constant 0.5125 nm.[27]

Liquid

[edit]

Liquid ammonia possesses strong ionising powers reflecting its high ε of 22 at −35 °C (−31 °F).[28] Liquid ammonia has a very high standard enthalpy change of vapourization (23.5 kJ/mol;[29] for comparison, water's is 40.65 kJ/mol, methane 8.19 kJ/mol and phosphine 14.6 kJ/mol) and can be transported in pressurized or refrigerated vessels; however, at standard temperature and pressure liquid anhydrous ammonia will vaporize.[30]

Solvent properties

[edit]

Ammonia readily dissolves in water. In an aqueous solution, it can be expelled by boiling. The aqueous solution of ammonia is basic, and may be described as aqueous ammonia or ammonium hydroxide.[31] The maximum concentration of ammonia in water (a saturated solution) has a specific gravity of 0.880 and is often known as '.880 ammonia'.[32]

Thermal and physical properties of saturated liquid ammonia[33][34]
Temperature
(°C)
Density
(kg/m3)
Specific heat
(kJ/(kg·K))
Kinematic
viscosity
(m2/s)
Thermal
conductivity
(W/(m·K))
Thermal
diffusivity
(m2/s)
Prandtl
Number
Bulk modulus
(K−1)
−50 703.69 4.463 4.35×10−7 0.547 1.74×10−7 2.6
−40 691.68 4.467 4.06×10−7 0.547 1.78×10−7 2.28
−30 679.34 4.476 3.87×10−7 0.549 1.80×10−7 2.15
−20 666.69 4.509 3.81×10−7 0.547 1.82×10−7 2.09
−10 653.55 4.564 3.78×10−7 0.543 1.83×10−7 2.07
0 640.1 4.635 3.73×10−7 0.540 1.82×10−7 2.05
10 626.16 4.714 3.68×10−7 0.531 1.80×10−7 2.04
20 611.75 4.798 3.59×10−7 0.521 1.78×10−7 2.02 2.45×10−3
30 596.37 4.89 3.49×10−7 0.507 1.74×10−7 2.01
40 580.99 4.999 3.40×10−7 0.493 1.70×10−7 2
50 564.33 5.116 3.30×10−7 0.476 1.65×10−7 1.99
Thermal and physical properties of ammonia (NH3) at atmospheric pressure[33][34]
Temperature
(K)
Temperature (°C) Density
(kg/m3)
Specific heat
(kJ/(kg·K))
Dynamic
viscosity
(kg/(m·s))
Kinematic
viscosity
(m2/s)
Thermal
conductivity
(W/(m·K))
Thermal
diffusivity
(m2/s)
Prandtl
Number
273 −0.15 0.7929 2.177 9.35×10−6 1.18×10−5 0.0220 1.31×10−5 0.90
323 49.85 0.6487 2.177 1.10×10−5 1.70×10−5 0.0270 1.92×10−5 0.88
373 99.85 0.559 2.236 1.29×10−5 1.30×10−5 0.0327 2.62×10−5 0.87
423 149.85 0.4934 2.315 1.47×10−5 2.97×10−5 0.0391 3.43×10−5 0.87
473 199.85 0.4405 2.395 1.65×10−5 3.74×10−5 0.0467 4.42×10−5 0.84
480 206.85 0.4273 2.43 1.67×10−5 3.90×10−5 0.0492 4.74×10−5 0.822
500 226.85 0.4101 2.467 1.73×10−5 4.22×10−5 0.0525 5.19×10−5 0.813
520 246.85 0.3942 2.504 1.80×10−5 4.57×10−5 0.0545 5.52×10−5 0.827
540 266.85 0.3795 2.54 1.87×10−5 4.91×10−5 0.0575 5.97×10−5 0.824
560 286.85 0.3708 2.577 1.93×10−5 5.20×10−5 0.0606 6.34×10−5 0.827
580 306.85 0.3533 2.613 2.00×10−5 5.65×10−5 0.0638 6.91×10−5 0.817

Liquid ammonia is a widely studied nonaqueous ionising solvent. Its most conspicuous property is its ability to dissolve alkali metals to form highly coloured, electrically conductive solutions containing solvated electrons. Apart from these remarkable solutions, much of the chemistry in liquid ammonia can be classified by analogy with related reactions in aqueous solutions. Comparison of the physical properties of NH3 with those of water shows NH3 has the lower melting point, boiling point, density, viscosity, dielectric constant and electrical conductivity. These differences are attributed at least in part to the weaker hydrogen bonding in NH3. The ionic self-dissociation constant of liquid NH3 at −50 °C is about 10−33.

A train carrying anhydrous ammonia
Solubility (g of salt per 100 g liquid NH3)
Ammonium acetate 253.2
Ammonium nitrate 389.6
Lithium nitrate 243.7
Sodium nitrate 97.6
Potassium nitrate 10.4
Sodium fluoride 0.35
Sodium chloride 157.0
Sodium bromide 138.0
Sodium iodide 161.9
Sodium thiocyanate 205.5

Liquid ammonia is an ionising solvent, although less so than water, and dissolves a range of ionic compounds, including many nitrates, nitrites, cyanides, thiocyanates, metal cyclopentadienyl complexes and metal bis(trimethylsilyl)amides.[33] Most ammonium salts are soluble and act as acids in liquid ammonia solutions. The solubility of halide salts increases from fluoride to iodide. A saturated solution of ammonium nitrate (Divers' solution, named after Edward Divers) contains 0.83 mol solute per mole of ammonia and has a vapour pressure of less than 1 bar even at 25 °C (77 °F). However, few oxyanion salts with other cations dissolve.[35]

Liquid ammonia will dissolve all of the alkali metals and other electropositive metals such as Ca,[36] Sr, Ba, Eu and Yb (also Mg using an electrolytic process[34]). At low concentrations (<0.06 mol/L), deep blue solutions are formed: these contain metal cations and solvated electrons, free electrons that are surrounded by a cage of ammonia molecules.

These solutions are strong reducing agents. At higher concentrations, the solutions are metallic in appearance and in electrical conductivity. At low temperatures, the two types of solution can coexist as immiscible phases.

Redox properties of liquid ammonia

[edit]
Liquid ammonia bottle
E° (V, ammonia) E° (V, water)
Li+ + e ⇌ Li −2.24 −3.04
K+ + e ⇌ K −1.98 −2.93
Na+ + e ⇌ Na −1.85 −2.71
Zn2+ + 2 e ⇌ Zn −0.53 −0.76
2 [NH4]+ + 2 e ⇌ H2 + 2 NH3 0.00
Cu2+ + 2 e ⇌ Cu +0.43 +0.34
Ag+ + e ⇌ Ag +0.83 +0.80

The range of thermodynamic stability of liquid ammonia solutions is very narrow, as the potential for oxidation to dinitrogen, E° (N2 + 6 [NH4]+ + 6 e ⇌ 8 NH3), is only +0.04 V. In practice, both oxidation to dinitrogen and reduction to dihydrogen are slow. This is particularly true of reducing solutions: the solutions of the alkali metals mentioned above are stable for several days, slowly decomposing to the metal amide and dihydrogen. Most studies involving liquid ammonia solutions are done in reducing conditions; although oxidation of liquid ammonia is usually slow, there is still a risk of explosion, particularly if transition metal ions are present as possible catalysts.

Structure

[edit]
Molecular structure of ammonia and its three-dimensional shape. It has a net dipole moment of 1.484 D.
Dot and cross structure of ammonia

The ammonia molecule has a trigonal pyramidal shape, as predicted by the valence shell electron pair repulsion theory (VSEPR theory) with an experimentally determined bond angle of 106.7°.[37] The central nitrogen atom has five outer electrons with an additional electron from each hydrogen atom. This gives a total of eight electrons, or four electron pairs that are arranged tetrahedrally. Three of these electron pairs are used as bond pairs, which leaves one lone pair of electrons. The lone pair repels more strongly than bond pairs; therefore, the bond angle is not 109.5°, as expected for a regular tetrahedral arrangement, but 106.7°.[37] This shape gives the molecule a dipole moment and makes it polar. The molecule's polarity, and especially its ability to form hydrogen bonds, makes ammonia highly miscible with water. The lone pair makes ammonia a base, a proton acceptor. Ammonia is moderately basic; a 1.0 M aqueous solution has a pH of 11.6, and if a strong acid is added to such a solution until the solution is neutral (pH = 7), 99.4% of the ammonia molecules are protonated. Temperature and salinity also affect the proportion of ammonium [NH4]+. The latter has the shape of a regular tetrahedron and is isoelectronic with methane.

The ammonia molecule readily undergoes nitrogen inversion at room temperature; a useful analogy is an umbrella turning itself inside out in a strong wind. The energy barrier to this inversion is 24.7 kJ/mol, and the resonance frequency is 23.79 GHz, corresponding to microwave radiation of a wavelength of 1.260 cm. The absorption at this frequency was the first microwave spectrum to be observed[38] and was used in the first maser.

Amphotericity

[edit]

One of the most characteristic properties of ammonia is its basicity. Ammonia is considered to be a weak base. It combines with acids to form ammonium salts; thus, with hydrochloric acid it forms ammonium chloride (sal ammoniac); with nitric acid, ammonium nitrate, etc. Perfectly dry ammonia gas will not combine with perfectly dry hydrogen chloride gas; moisture is necessary to bring about the reaction.[39][40]

As a demonstration experiment under air with ambient moisture, opened bottles of concentrated ammonia and hydrochloric acid solutions produce a cloud of ammonium chloride, which seems to appear 'out of nothing' as the salt aerosol forms where the two diffusing clouds of reagents meet between the two bottles.

NH3 + HCl → [NH4]Cl

The salts produced by the action of ammonia on acids are known as the ammonium salts and all contain the ammonium ion ([NH4]+).[39]

Although ammonia is well known as a weak base, it can also act as an extremely weak acid. It is a protic substance and is capable of formation of amides (which contain the NH2 ion). For example, lithium dissolves in liquid ammonia to give a blue solution (solvated electron) of lithium amide:

2 Li + 2 NH3 → 2 LiNH2 + H2

Self-dissociation

[edit]

Like water, liquid ammonia undergoes molecular autoionisation to form its acid and base conjugates:

2 NH3 ⇌ NH+4 + NH2

Ammonia often functions as a weak base, so it has some buffering ability. Shifts in pH will cause more or fewer ammonium cations (NH+4) and amide anions (NH2) to be present in solution. At standard pressure and temperature,

K = [NH+4] × [NH2] = 10−30.

Combustion

[edit]
Heated Cr2O3 catalyzes the combustion of a flask of ammonia.

Ammonia does not burn readily or sustain combustion, except under narrow fuel-to-air mixtures of 15–28% ammonia by volume in air.[41] When mixed with oxygen, it burns with a pale yellowish-green flame. Ignition occurs when chlorine is passed into ammonia, forming nitrogen and hydrogen chloride; if chlorine is present in excess, then the highly explosive nitrogen trichloride (NCl3) is also formed.

The combustion of ammonia to form nitrogen and water is exothermic:

4 NH3 + 3 O2 → 2 N2 + 6 H2O(g), ΔH°r = −1267.20 kJ (or −316.8 kJ/mol if expressed per mol of NH3)

The standard enthalpy change of combustion, ΔH°c, expressed per mole of ammonia and with condensation of the water formed, is −382.81 kJ/mol. Dinitrogen is the thermodynamic product of combustion: all nitrogen oxides are unstable with respect to N2 and O2, which is the principle behind the catalytic converter. Nitrogen oxides can be formed as kinetic products in the presence of appropriate catalysts, a reaction of great industrial importance in the production of nitric acid:

4 NH3 + 5 O2 → 4 NO + 6 H2O

A subsequent reaction leads to NO2:

2 NO + O2 → 2 NO2

The combustion of ammonia in air is very difficult in the absence of a catalyst (such as platinum gauze or warm chromium(III) oxide), due to the relatively low heat of combustion, a lower laminar burning velocity, high auto-ignition temperature, high heat of vapourization, and a narrow flammability range. However, recent studies have shown that efficient and stable combustion of ammonia can be achieved using swirl combustors, thereby rekindling research interest in ammonia as a fuel for thermal power production.[42] The flammable range of ammonia in dry air is 15.15–27.35% and in 100% relative humidity air is 15.95–26.55%.[43][clarification needed] For studying the kinetics of ammonia combustion, knowledge of a detailed reliable reaction mechanism is required, but this has been challenging to obtain.[44]

Precursor to organonitrogen compounds

[edit]

Ammonia is a direct or indirect precursor to most manufactured nitrogen-containing compounds. It is the precursor to nitric acid, which is the source for most N-substituted aromatic compounds.

Amines can be formed by the reaction of ammonia with alkyl halides or, more commonly, with alcohols:

CH3OH + NH3 → CH3NH2 + H2O

Its ring-opening reaction with ethylene oxide give ethanolamine, diethanolamine, and triethanolamine.

Amides can be prepared by the reaction of ammonia with carboxylic acid and their derivatives. For example, ammonia reacts with formic acid (HCOOH) to yield formamide (HCONH2) when heated. Acyl chlorides are the most reactive, but the ammonia must be present in at least a twofold excess to neutralise the hydrogen chloride formed. Esters and anhydrides also react with ammonia to form amides. Ammonium salts of carboxylic acids can be dehydrated to amides by heating to 150–200 °C as long as no thermally sensitive groups are present.

Other organonitrogen compounds include alprazolam, ethanolamine, ethyl carbamate and hexamethylenetetramine.

Precursor to inorganic nitrogenous compounds

[edit]

Nitric acid is generated via the Ostwald process by oxidation of ammonia with air over a platinum catalyst at 700–850 °C (1,292–1,562 °F), ≈9 atm. Nitric oxide and nitrogen dioxide are intermediate in this conversion:[45]

NH3 + 2 O2 → HNO3 + H2O

Nitric acid is used for the production of fertilisers, explosives, and many organonitrogen compounds.

The hydrogen in ammonia is susceptible to replacement by a myriad substituents. Ammonia gas reacts with metallic sodium to give sodamide, NaNH2.[39]

With chlorine, monochloramine is formed.

Pentavalent ammonia is known as λ5-amine, nitrogen pentahydride decomposes spontaneously into trivalent ammonia (λ3-amine) and hydrogen gas at normal conditions. This substance was once investigated as a possible solid rocket fuel in 1966.[46]

Ammonia is also used to make the following compounds:

Cisplatin ([Pt(NH3)2Cl2) is a widely used anticancer drug.

Ammonia is a ligand forming metal ammine complexes. For historical reasons, ammonia is named ammine in the nomenclature of coordination compounds. One notable ammine complex is cisplatin (Pt(NH3)2Cl2, a widely used anticancer drug. Ammine complexes of chromium(III) formed the basis of Alfred Werner's revolutionary theory on the structure of coordination compounds. Werner noted only two isomers (fac- and mer-) of the complex [CrCl3(NH3)3] could be formed, and concluded the ligands must be arranged around the metal ion at the vertices of an octahedron.

Ammonia forms 1:1 adducts with a variety of Lewis acids such as I2, phenol, and Al(CH3)3. Ammonia is a hard base (HSAB theory) and its E & C parameters are EB = 2.31 and CB = 2.04. Its relative donor strength toward a series of acids, versus other Lewis bases, can be illustrated by C-B plots.

Detection and determination

[edit]

Ammonia in solution

[edit]

Ammonia and ammonium salts can be readily detected, in very minute traces, by the addition of Nessler's solution, which gives a distinct yellow colouration in the presence of the slightest trace of ammonia or ammonium salts. The amount of ammonia in ammonium salts can be estimated quantitatively by distillation of the salts with sodium (NaOH) or potassium hydroxide (KOH), the ammonia evolved being absorbed in a known volume of standard sulfuric acid and the excess of acid then determined volumetrically; or the ammonia may be absorbed in hydrochloric acid and the ammonium chloride so formed precipitated as ammonium hexachloroplatinate, [NH4]2[PtCl6].[47]

Gaseous ammonia

[edit]

Sulfur sticks are burnt to detect small leaks in industrial ammonia refrigeration systems. Larger quantities can be detected by warming the salts with a caustic alkali or with quicklime, when the characteristic smell of ammonia will be at once apparent.[47] Ammonia is an irritant and irritation increases with concentration; the permissible exposure limit is 25 ppm, and lethal above 500 ppm by volume.[48] Higher concentrations are hardly detected by conventional detectors, the type of detector is chosen according to the sensitivity required (e.g. semiconductor, catalytic, electrochemical). Holographic sensors have been proposed for detecting concentrations up to 12.5% in volume.[49]

In a laboratorial setting, gaseous ammonia can be detected by using concentrated hydrochloric acid or gaseous hydrogen chloride. A dense white fume (which is ammonium chloride vapor) arises from the reaction between ammonia and HCl(g).[50]

Ammoniacal nitrogen (NH3–N)

[edit]

Ammoniacal nitrogen (NH3–N) is a measure commonly used for testing the quantity of ammonium ions, derived naturally from ammonia, and returned to ammonia via organic processes, in water or waste liquids. It is a measure used mainly for quantifying values in waste treatment and water purification systems, as well as a measure of the health of natural and man-made water reserves. It is measured in units of mg/L (milligram per litre).

History

[edit]
Jabir ibn Hayyan wrote about ammonia in the 9th century
This high-pressure ammonia reactor was built in 1921 by BASF in Ludwigshafen and was re-erected on the premises of the University of Karlsruhe in Germany.

The ancient Greek historian Herodotus mentioned that there were outcrops of salt in an area of Libya that was inhabited by a people called the 'Ammonians' (now the Siwa oasis in northwestern Egypt, where salt lakes still exist).[51][52] The Greek geographer Strabo also mentioned the salt from this region. However, the ancient authors Dioscorides, Apicius, Arrian, Synesius, and Aëtius of Amida described this salt as forming clear crystals that could be used for cooking and that were essentially rock salt.[53] Hammoniacus sal appears in the writings of Pliny,[54] although it is not known whether the term is equivalent to the more modern sal ammoniac (ammonium chloride).[22][55][56]

The fermentation of urine by bacteria produces a solution of ammonia; hence fermented urine was used in Classical Antiquity to wash cloth and clothing, to remove hair from hides in preparation for tanning, to serve as a mordant in dyeing cloth, and to remove rust from iron.[57] It was also used by ancient dentists to wash teeth.[58][59][60]

In the form of sal ammoniac (نشادر, nushadir), ammonia was important to the Muslim alchemists. It was mentioned in the Book of Stones, likely written in the 9th century and attributed to Jābir ibn Hayyān.[61] It was also important to the European alchemists of the 13th century, being mentioned by Albertus Magnus.[22] It was also used by dyers in the Middle Ages in the form of fermented urine to alter the colour of vegetable dyes. In the 15th century, Basilius Valentinus showed that ammonia could be obtained by the action of alkalis on sal ammoniac.[62] At a later period, when sal ammoniac was obtained by distilling the hooves and horns of oxen and neutralizing the resulting carbonate with hydrochloric acid, the name 'spirit of hartshorn' was applied to ammonia.[22][63]

Gaseous ammonia was first isolated by Joseph Black in 1756 by reacting sal ammoniac (ammonium chloride) with calcined magnesia (magnesium oxide).[64][65] It was isolated again by Peter Woulfe in 1767,[66][67] by Carl Wilhelm Scheele in 1770[68] and by Joseph Priestley in 1773 and was termed by him 'alkaline air'.[22][69] Eleven years later in 1785, Claude Louis Berthollet ascertained its composition.[70][22]

The production of ammonia from nitrogen in the air (and hydrogen) was invented by Fritz Haber and Robert LeRossignol. The patent was sent in 1909 (USPTO Nr 1,202,995) and awarded in 1916. Later, Carl Bosch developed the industrial method for ammonia production (Haber–Bosch process). It was first used on an industrial scale in Germany during World War I,[71] following the allied blockade that cut off the supply of nitrates from Chile. The ammonia was used to produce explosives to sustain war efforts.[72] The Nobel Prize in Chemistry 1918 was awarded to Fritz Haber "for the synthesis of ammonia from its elements".

Before the availability of natural gas, hydrogen as a precursor to ammonia production was produced via the electrolysis of water or using the chloralkali process.

With the advent of the steel industry in the 20th century, ammonia became a byproduct of the production of coking coal.

Applications

[edit]

Fertilizer

[edit]

In the US as of 2019, approximately 88% of ammonia was used as fertilizers either as its salts, solutions or anhydrously.[73] When applied to soil, it helps provide increased yields of crops such as maize and wheat.[74] 30% of agricultural nitrogen applied in the US is in the form of anhydrous ammonia, and worldwide, 110 million tonnes are applied each year.[75] Solutions of ammonia ranging from 16% to 25% are used in the fermentation industry as a source of nitrogen for microorganisms and to adjust pH during fermentation.[76]

Refrigeration–R717

[edit]

Because of ammonia's vapourization properties, it is a useful refrigerant.[71] It was commonly used before the popularisation of chlorofluorocarbons (Freons). Anhydrous ammonia is widely used in industrial refrigeration applications and hockey rinks because of its high energy efficiency and low cost. It suffers from the disadvantage of toxicity, and requiring corrosion resistant components, which restricts its domestic and small-scale use. Along with its use in modern vapour-compression refrigeration it is used in a mixture along with hydrogen and water in absorption refrigerators. The Kalina cycle, which is of growing importance to geothermal power plants, depends on the wide boiling range of the ammonia–water mixture.

Ammonia coolant is also used in the radiators aboard the International Space Station in loops that are used to regulate the internal temperature and enable temperature-dependent experiments.[77][78] The ammonia is under sufficient pressure to remain liquid throughout the process. Single-phase ammonia cooling systems also serve the power electronics in each pair of solar arrays.

The potential importance of ammonia as a refrigerant has increased with the discovery that vented CFCs and HFCs are potent and stable greenhouse gases.[79]

Antimicrobial agent for food products

[edit]

As early as in 1895, it was known that ammonia was 'strongly antiseptic; it requires 1.4 grams per litre to preserve beef tea (broth).'[80] In one study, anhydrous ammonia destroyed 99.999% of zoonotic bacteria in three types of animal feed, but not silage.[81][82] Anhydrous ammonia is currently used commercially to reduce or eliminate microbial contamination of beef.[83][84] Lean finely textured beef (popularly known as 'pink slime') in the beef industry is made from fatty beef trimmings (c. 50–70% fat) by removing the fat using heat and centrifugation, then treating it with ammonia to kill E. coli. The process was deemed effective and safe by the US Department of Agriculture based on a study that found that the treatment reduces E. coli to undetectable levels.[85] There have been safety concerns about the process as well as consumer complaints about the taste and smell of ammonia-treated beef.[86]

Fuel

[edit]
Ammoniacal Gas Engine Streetcar in New Orleans drawn by Alfred Waud in 1871

Ammonia has been used as fuel, and is a proposed alternative to fossil fuels and hydrogen, especially in maritime transport. Being liquid at ambient temperature under its own vapour pressure and having high volumetric and gravimetric energy density, ammonia is considered a suitable carrier for hydrogen,[87] and may be cheaper than direct transport of liquid hydrogen.[88]

Compared to hydrogen, ammonia is easier to store. Compared to hydrogen as a fuel, ammonia is much more energy efficient, and could be produced, stored and delivered at a much lower cost than hydrogen, which must be kept compressed or as a cryogenic liquid.[89][90] The raw energy density of liquid ammonia is 11.5 MJ/L,[89] which is about a third that of diesel. Ammonia can also be converted back to hydrogen to be used to power hydrogen fuel cells, or it may be used directly within high-temperature solid oxide direct ammonia fuel cells to provide efficient power sources that do not emit greenhouse gases.[91][92] Ammonia to hydrogen conversion can be achieved through the sodium amide process[93] or the catalytic decomposition of ammonia using solid catalysts.[94]

Ammonia production currently creates 1.8% of global CO2 emissions. 'Green ammonia' is ammonia produced by using green hydrogen (hydrogen produced by electrolysis with electricity from renewable energy), whereas 'blue ammonia' is ammonia produced using blue hydrogen (hydrogen produced by steam methane reforming) where the carbon dioxide has been captured and stored.[95] In a world first in 2020, Saudi Arabia shipped 40 metric tons of liquid 'blue ammonia' to Japan for use as a fuel.[96] It was produced as a by-product by petrochemical industries, and can be burned without giving off greenhouse gases. Its energy density by volume is nearly double that of liquid hydrogen. If the process of creating it can be scaled up via purely renewable resources, producing green ammonia, it could make a major difference in avoiding climate change.[97]

Ships and maritime transport

[edit]

Green ammonia is considered as a potential fuel for new ships, including future container ships. Ammonia is expected to increase in usage as a fuel source for shipping [98] The IEA forecasts that ammonia will meet approximately 45% of shipping fuel demands by 2050.[99]

In 2020, the companies DSME and MAN Energy Solutions announced the construction of an ammonia-based ship, DSME plans to commercialize it by 2025.[100] The use of ammonia as a potential alternative fuel for aircraft jet engines is also being explored.[101] In addition, hybrid engine configurations for supersonic aviation employing ammonia fuel have been investigated. [102] Japan is implementing a plan to develop ammonia co-firing technology that can increase the use of ammonia in power generation, as part of efforts to assist domestic and other Asian utilities to accelerate their transition to carbon neutrality.[103] In October 2021, the first International Conference on Fuel Ammonia (ICFA2021) was held.[104][105]

In June 2022, IHI Corporation succeeded in reducing greenhouse gases by over 99% during combustion of liquid ammonia in a 2,000-kilowatt-class gas turbine achieving truly CO2-free power generation.[106] In July 2022, Quad nations of Japan, the U.S., Australia and India agreed to promote technological development for clean-burning hydrogen and ammonia as fuels at the security grouping's first energy meeting.[107] As of 2022, however, significant amounts of NOx are produced.[108] Nitrous oxide may also be a problem as it is a "greenhouse gas that is known to possess up to 300 times the Global Warming Potential (GWP) of carbon dioxide".[109]

Vehicles, aviation and space

[edit]
The X-15 aircraft used ammonia as one component fuel of its rocket engine

Ammonia engines or ammonia motors, using ammonia as a working fluid, have been proposed and occasionally used.[110] The principle is similar to that used in a fireless locomotive, but with ammonia as the working fluid, instead of steam or compressed air. Ammonia engines were used experimentally in the 19th century by Goldsworthy Gurney in the UK and the St. Charles Streetcar Line in New Orleans in the 1870s and 1880s,[111] and during World War II ammonia was used to power buses in Belgium.[112]

Ammonia is sometimes proposed as a practical alternative to fossil fuel for internal combustion engines.[112][113][114][115] However, ammonia cannot be easily used in existing Otto cycle engines because of its very narrow flammability range. Despite this, several tests have been run.[116][117][118] Its high octane rating of 120[119] and low flame temperature[120] allows the use of high compression ratios without a penalty of high NOx production. Since ammonia contains no carbon, its combustion cannot produce carbon dioxide, carbon monoxide, hydrocarbons, or soot. At high temperature and in the presence of a suitable catalyst ammonia decomposes into its constituent elements.[121] Decomposition of ammonia is a slightly endothermic process requiring 23 kJ/mol (5.5 kcal/mol) of ammonia, and yields hydrogen and nitrogen gas.

Rocket engines have also been fueled by ammonia. The Reaction Motors XLR99 rocket engine that powered the X-15 hypersonic research aircraft used liquid ammonia. Although not as powerful as other fuels, it left no soot in the reusable rocket engine, and its density approximately matches the density of the oxidiser, liquid oxygen, which simplified the aircraft's design.

Power stations

[edit]

The company ACWA Power and the city of Neom have announced the construction of a green hydrogen and ammonia plant in 2020.[122]

Other

[edit]

Remediation of gaseous emissions

[edit]

Ammonia is used to scrub SO2 from the burning of fossil fuels, and the resulting product is converted to ammonium sulfate for use as fertiliser. Ammonia neutralises the nitrogen oxide (NOx) pollutants emitted by diesel engines. This technology, called SCR (selective catalytic reduction), relies on a vanadia-based catalyst.[123]

Ammonia may be used to mitigate gaseous spills of phosgene.[124]

Stimulant

[edit]
Anti-meth sign on tank of anhydrous ammonia, Otley, Iowa. Anhydrous ammonia is a common farm fertiliser that is also a critical ingredient in making methamphetamine. In 2005, Iowa used grant money to provide thousands of locks to prevent criminals from gaining access to the tanks.[125]

Ammonia, as the vapour released by smelling salts, has found significant use as a respiratory stimulant. Ammonia is commonly used in the illegal manufacture of methamphetamine through a Birch reduction.[126] The Birch method of making methamphetamine is dangerous because the alkali metal and liquid ammonia are both extremely reactive, and the temperature of liquid ammonia makes it susceptible to explosive boiling when reactants are added.[127]

Textile

[edit]

Liquid ammonia is used for treatment of cotton materials, giving properties like mercerisation, using alkalis. In particular, it is used for prewashing of wool.[128]

Lifting gas

[edit]

At standard temperature and pressure, ammonia is less dense than atmosphere and has approximately 45–48% of the lifting power of hydrogen or helium. Ammonia has sometimes been used to fill balloons as a lifting gas. Because of its relatively high boiling point (compared to helium and hydrogen), ammonia could potentially be refrigerated and liquefied aboard an airship to reduce lift and add ballast (and returned to a gas to add lift and reduce ballast).[129]

Fuming

[edit]

Ammonia has been used to darken quartersawn white oak in Arts & Crafts and Mission-style furniture. Ammonia fumes react with the natural tannins in the wood and cause it to change colour.[130]

Cleaning agent

[edit]

Ammonia is used as an ingredient in various cleaning products, such as Windex (until 2006), in the form of ammonia solution.

Safety

[edit]
The world's longest ammonia pipeline (roughly 2400 km long),[131] running from the TogliattiAzot plant in Russia to Odesa in Ukraine

The US Occupational Safety and Health Administration (OSHA) has set a 15-minute exposure limit for gaseous ammonia of 35 ppm by volume in the environmental air and an 8-hour exposure limit of 25 ppm by volume.[132] The National Institute for Occupational Safety and Health (NIOSH) recently reduced the IDLH (Immediately Dangerous to Life or Health, the level to which a healthy worker can be exposed for 30 minutes without suffering irreversible health effects) from 500 to 300 ppm based on recent more conservative interpretations of original research in 1943. Other organisations have varying exposure levels. US Navy Standards [U.S. Bureau of Ships 1962] maximum allowable concentrations (MACs): for continuous exposure (60 days) is 25 ppm; for exposure of 1 hour is 400 ppm.[133]

Ammonia vapour has a sharp, irritating, pungent odor that acts as a warning of potentially dangerous exposure. The average odor threshold is 5 ppm, well below any danger or damage. Exposure to very high concentrations of gaseous ammonia can result in lung damage and death.[132] Ammonia is regulated in the US as a non-flammable gas, but it meets the definition of a material that is toxic by inhalation and requires a hazardous safety permit when transported in quantities greater than 3,500 US gallons (13,000 L; 2,900 imp gal).[134]

Liquid ammonia is dangerous because it is hygroscopic and because it can cause caustic burns. See Gas carrier § Health effects of specific cargoes carried on gas carriers for more information.

Toxicity

[edit]

The toxicity of ammonia solutions does not usually cause problems for humans and other mammals, as a specific mechanism exists to prevent its build-up in the bloodstream. Ammonia is converted to carbamoyl phosphate by the enzyme carbamoyl phosphate synthetase, and then enters the urea cycle to be either incorporated into amino acids or excreted in the urine.[135] Fish and amphibians lack this mechanism, as they can usually eliminate ammonia from their bodies by direct excretion. Ammonia even at dilute concentrations is highly toxic to aquatic animals, and for this reason it is classified as "dangerous for the environment". Atmospheric ammonia plays a key role in the formation of fine particulate matter.[136]

Ammonia is a constituent of tobacco smoke.[137]

Coking wastewater

[edit]

Ammonia is present in coking wastewater streams, as a liquid by-product of the production of coke from coal.[138] In some cases, the ammonia is discharged to the marine environment where it acts as a pollutant. The Whyalla Steelworks in South Australia is one example of a coke-producing facility that discharges ammonia into marine waters.[139]

Aquaculture

[edit]

Ammonia toxicity is believed to be a cause of otherwise unexplained losses in fish hatcheries. Excess ammonia may accumulate and cause alteration of metabolism or increases in the body pH of the exposed organism. Tolerance varies among fish species.[140] At lower concentrations, around 0.05 mg/L, un-ionised ammonia is harmful to fish species and can result in poor growth and feed conversion rates, reduced fecundity and fertility and increase stress and susceptibility to bacterial infections and diseases.[141] Exposed to excess ammonia, fish may suffer loss of equilibrium, hyper-excitability, increased respiratory activity and oxygen uptake and increased heart rate.[140] At concentrations exceeding 2.0 mg/L, ammonia causes gill and tissue damage, extreme lethargy, convulsions, coma, and death.[140][142] Experiments have shown that the lethal concentration for a variety of fish species ranges from 0.2 to 2.0 mg/L.[142]

During winter, when reduced feeds are administered to aquaculture stock, ammonia levels can be higher. Lower ambient temperatures reduce the rate of algal photosynthesis so less ammonia is removed by any algae present. Within an aquaculture environment, especially at large scale, there is no fast-acting remedy to elevated ammonia levels. Prevention rather than correction is recommended to reduce harm to farmed fish[142] and in open water systems, the surrounding environment.

Storage information

[edit]

Similar to propane, anhydrous ammonia boils below room temperature when at atmospheric pressure. A storage vessel capable of 250 psi (1.7 MPa) is suitable to contain the liquid.[143] Ammonia is used in numerous different industrial applications requiring carbon or stainless steel storage vessels. Ammonia with at least 0.2% by weight water content is not corrosive to carbon steel. NH3 carbon steel construction storage tanks with 0.2% by weight or more of water could last more than 50 years in service.[144] Experts warn that ammonium compounds not be allowed to come in contact with bases (unless in an intended and contained reaction), as dangerous quantities of ammonia gas could be released.

Laboratory

[edit]
A standard laboratory solution of 28% ammonia

The hazards of ammonia solutions depend on the concentration: 'dilute' ammonia solutions are usually 5–10% by weight (< 5.62 mol/L); 'concentrated' solutions are usually prepared at >25% by weight. A 25% (by weight) solution has a density of 0.907 g/cm3, and a solution that has a lower density will be more concentrated. The European Union classification of ammonia solutions is given in the table.

Concentration
by weight (w/w)
Molarity Concentration
mass/volume (w/v)
GHS pictograms H-phrases
5–10% 2.87–5.62 mol/L 48.9–95.7 g/L GHS07: Exclamation mark H314
10–25% 5.62–13.29 mol/L 95.7–226.3 g/L GHS05: CorrosiveGHS07: Exclamation mark H314, H335, H400
>25% >13.29 mol/L >226.3 g/L GHS05: CorrosiveGHS07: Exclamation markGHS09: Environmental hazard H314, H335, H400, H411

The ammonia vapour from concentrated ammonia solutions is severely irritating to the eyes and the respiratory tract, and experts warn that these solutions only be handled in a fume hood. Saturated ('0.880'–see § Properties) solutions can develop a significant pressure inside a closed bottle in warm weather, and experts also warn that the bottle be opened with care. This is not usually a problem for 25% ('0.900') solutions.

Experts warn that ammonia solutions not be mixed with halogens, as toxic and/or explosive products are formed. Experts also warn that prolonged contact of ammonia solutions with silver, mercury or iodide salts can also lead to explosive products: such mixtures are often formed in qualitative inorganic analysis, and that it needs to be lightly acidified but not concentrated (<6% w/v) before disposal once the test is completed.

Laboratory use of anhydrous ammonia (gas or liquid)

[edit]

Anhydrous ammonia is classified as toxic (T) and dangerous for the environment (N). The gas is flammable (autoignition temperature: 651 °C) and can form explosive mixtures with air (16–25%). The permissible exposure limit (PEL) in the United States is 50 ppm (35 mg/m3), while the IDLH concentration is estimated at 300 ppm. Repeated exposure to ammonia lowers the sensitivity to the smell of the gas: normally the odour is detectable at concentrations of less than 50 ppm, but desensitised individuals may not detect it even at concentrations of 100 ppm. Anhydrous ammonia corrodes copper- and zinc-containing alloys, which makes brass fittings not appropriate for handling the gas. Liquid ammonia can also attack rubber and certain plastics.

Ammonia reacts violently with the halogens. Nitrogen triiodide, a primary high explosive, is formed when ammonia comes in contact with iodine. Ammonia causes the explosive polymerisation of ethylene oxide. It also forms explosive fulminating compounds with compounds of gold, silver, mercury, germanium or tellurium, and with stibine. Violent reactions have also been reported with acetaldehyde, hypochlorite solutions, potassium ferricyanide and peroxides.

Production

[edit]
Year030K60K90K120K150K19501960197019801990200020102020World production in thousands of tons of fixed nitrogenGlobal ammonia production since 1950 (fixed ...
Global ammonia production 1950–2020 (expressed as fixed nitrogen in U.S. tons)[145]

Ammonia has one of the highest rates of production of any inorganic chemical. Production is sometimes expressed in terms of "fixed nitrogen". Global production was estimated as being 160 million tonnes in 2020 (147 tons of fixed nitrogen).[146] China accounted for 26.5% of that, followed by Russia at 11.0%, the United States at 9.5%, and India at 8.3%.[146]

Before the start of World War I, most ammonia was obtained by the dry distillation[147] of nitrogenous vegetable and animal waste products, including camel dung, where it was distilled by the reduction of nitrous acid and nitrites with hydrogen; in addition, it was produced by the distillation of coal, and also by the decomposition of ammonium salts by alkaline hydroxides[148] such as quicklime:[22]

2 [NH4]Cl + 2 CaO → CaCl2 + Ca(OH)2 + 2 NH3(g)

For small scale laboratory synthesis, one can heat urea and calcium hydroxide or sodium hydroxide:

(NH2)2CO + Ca(OH)2 → CaCO3 + 2 NH3

Haber–Bosch

[edit]
Fritz Haber, 1918

The Haber process,[149] also called the Haber–Bosch process, is the main industrial procedure for the production of ammonia.[150][151] It converts atmospheric nitrogen (N2) to ammonia (NH3) by a reaction with hydrogen (H2) using finely divided iron metal as a catalyst:

This reaction is exothermic but disfavored in terms of entropy because four equivalents of reactant gases are converted into two equivalents of product gas. As a result, sufficiently high pressures and temperatures are needed to drive the reaction forward.

The German chemists Fritz Haber and Carl Bosch developed the process in the first decade of the 20th century, and its improved efficiency over existing methods such as the Birkeland-Eyde and Frank-Caro processes was a major advancement in the industrial production of ammonia.[152][153][154]

The Haber process can be combined with steam reforming to produce ammonia with just three chemical inputs: water, natural gas, and atmospheric nitrogen. Both Haber and Bosch were eventually awarded the Nobel Prize in Chemistry: Haber in 1918 for ammonia synthesis specifically, and Bosch in 1931 for related contributions to high-pressure chemistry.

Electrochemical

[edit]

The electrochemical synthesis of ammonia involves the reductive formation of lithium nitride, which can be protonated to ammonia, given a proton source. The first use of this chemistry was reported in 1930, where lithium solutions in ethanol were used to produce ammonia at pressures of up to 1000 bar, with ethanol acting as the proton source.[155] Beyond simply mediating proton transfer to the nitrogen reduction reaction, ethanol has been found to play a multifaceted role, influencing electrolyte transformations and contributing to the formation of the solid electrolyte interphase, which enhances overall reaction efficiency.[156][157]

In 1994, Tsuneto et al. used lithium electrodeposition in tetrahydrofuran to synthesize ammonia at more moderate pressures with reasonable Faradaic efficiency.[158] Subsequent studies have further explored the ethanol–tetrahydrofuran system for electrochemical ammonia synthesis.[157][159]

In 2020, a solvent-agnostic gas diffusion electrode was shown to improve nitrogen transport to the reactive lithium. NH3 production rates of up to 30 ± 5 nmol/(s⋅cm2) and Faradaic efficiencies of up to 47.5 ± 4% at ambient temperature and 1 bar pressure were achieved.[160]

In 2021, it was demonstrated that ethanol could be replaced with a tetraalkyl phosphonium salt.[161] The study observed NH3 production rates of 53 ± 1 nmol/(s⋅cm2) at 69 ± 1% Faradaic efficiency experiments under 0.5 bar hydrogen and 19.5 bar nitrogen partial pressure at ambient temperature.[161] Technology based on this electrochemistry is being developed for commercial fertiliser and fuel production.[162][163]

In 2022, ammonia was produced via the lithium mediated process in a continuous-flow electrolyzer also demonstrating the hydrogen gas as proton source. The study synthesized ammonia at 61 ± 1% Faradaic efficiency at a current density of −6 mA/cm2 at 1 bar and room temperature.[164]

Biochemistry and medicine

[edit]
Main symptoms of hyperammonemia (ammonia reaching toxic concentrations).[165]

Ammonia is essential for life.[166] For example, it is required for the formation of amino acids and nucleic acids, fundamental building blocks of life. Ammonia is however quite toxic. Nature thus uses carriers for ammonia. Within a cell, glutamate serves this role. In the bloodstream, glutamine is a source of ammonia.[167]

Ethanolamine, required for cell membranes, is the substrate for ethanolamine ammonia-lyase, which produces ammonia:[168]

H2NCH2CH2OH → NH3 + CH3CHO

Ammonia is both a metabolic waste and a metabolic input throughout the biosphere. It is an important source of nitrogen for living systems. Although atmospheric nitrogen abounds (more than 75%), few living creatures are capable of using atmospheric nitrogen in its diatomic form, N2 gas. Therefore, nitrogen fixation is required for the synthesis of amino acids, which are the building blocks of protein. Some plants rely on ammonia and other nitrogenous wastes incorporated into the soil by decaying matter. Others, such as nitrogen-fixing legumes, benefit from symbiotic relationships with rhizobia bacteria that create ammonia from atmospheric nitrogen.[169]

In humans, inhaling ammonia in high concentrations can be fatal. Exposure to ammonia can cause headaches, edema, impaired memory, seizures and coma as it is neurotoxic in nature.[170]

Biosynthesis

[edit]

In certain organisms, ammonia is produced from atmospheric nitrogen by enzymes called nitrogenases. The overall process is called nitrogen fixation. Intense effort has been directed toward understanding the mechanism of biological nitrogen fixation. The scientific interest in this problem is motivated by the unusual structure of the active site of the enzyme, which consists of an Fe7MoS9 ensemble.[171]

Ammonia is also a metabolic product of amino acid deamination catalyzed by enzymes such as glutamate dehydrogenase 1. Ammonia excretion is common in aquatic animals. In humans, it is quickly converted to urea (by liver), which is much less toxic, particularly less basic. This urea is a major component of the dry weight of urine. Most reptiles, birds, insects, and snails excrete uric acid solely as nitrogenous waste.

Physiology

[edit]

Ammonia plays a role in both normal and abnormal animal physiology. It is biosynthesised through normal amino acid metabolism and is toxic in high concentrations. The liver converts ammonia to urea through a series of reactions known as the urea cycle. Liver dysfunction, such as that seen in cirrhosis, may lead to elevated amounts of ammonia in the blood (hyperammonemia). Likewise, defects in the enzymes responsible for the urea cycle, such as ornithine transcarbamylase, lead to hyperammonemia. Hyperammonemia contributes to the confusion and coma of hepatic encephalopathy, as well as the neurological disease common in people with urea cycle defects and organic acidurias.[172]

Ammonia is important for normal animal acid/base balance. After formation of ammonium from glutamine, α-ketoglutarate may be degraded to produce two bicarbonate ions, which are then available as buffers for dietary acids. Ammonium is excreted in the urine, resulting in net acid loss. Ammonia may itself diffuse across the renal tubules, combine with a hydrogen ion, and thus allow for further acid excretion.[173]

Excretion

[edit]

Ammonium ions are a toxic waste product of metabolism in animals. In fish and aquatic invertebrates, it is excreted directly into the water. In mammals, sharks, and amphibians, it is converted in the urea cycle to urea, which is less toxic and can be stored more efficiently. In birds, reptiles, and terrestrial snails, metabolic ammonium is converted into uric acid, which is solid and can therefore be excreted with minimal water loss.[174]

Extraterrestrial occurrence

[edit]
Ammonia occurs in the atmospheres of the outer giant planets such as Jupiter (0.026% ammonia), Saturn (0.012% ammonia), and in the atmospheres and ices of Uranus and Neptune.

Ammonia has been detected in the atmospheres of the giant planets Jupiter, Saturn, Uranus and Neptune, along with other gases such as methane, hydrogen, and helium. The interior of Saturn may include frozen ammonia crystals.[175]

Interstellar space

[edit]

Ammonia was first detected in interstellar space in 1968, based on microwave emissions from the direction of the galactic core.[176] This was the first polyatomic molecule to be so detected. The sensitivity of the molecule to a broad range of excitations and the ease with which it can be observed in a number of regions has made ammonia one of the most important molecules for studies of molecular clouds.[177] The relative intensity of the ammonia lines can be used to measure the temperature of the emitting medium.

The following isotopic species of ammonia have been detected: NH3,15NH3, NH2D, NHD2, and ND3. The detection of triply deuterated ammonia was considered a surprise as deuterium is relatively scarce. It is thought that the low-temperature conditions allow this molecule to survive and accumulate.[178]

Since its interstellar discovery, NH3 has proved to be an invaluable spectroscopic tool in the study of the interstellar medium. With a large number of transitions sensitive to a wide range of excitation conditions, NH3 has been widely astronomically detected–its detection has been reported in hundreds of journal articles. Listed below is a sample of journal articles that highlights the range of detectors that have been used to identify ammonia.

The study of interstellar ammonia has been important to a number of areas of research in the last few decades. Some of these are delineated below and primarily involve using ammonia as an interstellar thermometer.

Interstellar formation mechanisms

[edit]

The interstellar abundance for ammonia has been measured for a variety of environments. The [NH3]/[H2] ratio has been estimated to range from 10−7 in small dark clouds[179] up to 10−5 in the dense core of the Orion molecular cloud complex.[180] Although a total of 18 total production routes have been proposed,[181] the principal formation mechanism for interstellar NH3 is the reaction:

[NH4]+ + e → NH3 + H

The rate constant, k, of this reaction depends on the temperature of the environment, with a value of at 10 K.[182] The rate constant was calculated from the formula . For the primary formation reaction, a = 1.05×10−6 and B = −0.47. Assuming an NH+4 abundance of and an electron abundance of 10−7 typical of molecular clouds, the formation will proceed at a rate of 1.6×10−9 cm−3s−1 in a molecular cloud of total density 105 cm−3.[183]

All other proposed formation reactions have rate constants of between two and 13 orders of magnitude smaller, making their contribution to the abundance of ammonia relatively insignificant.[184] As an example of the minor contribution other formation reactions play, the reaction:

H2 + NH2 → NH3 + H

has a rate constant of 2.2×10−15. Assuming H2 densities of 105 and [NH2]/[H2] ratio of 10−7, this reaction proceeds at a rate of 2.2×10−12, more than three orders of magnitude slower than the primary reaction above.

Some of the other possible formation reactions are:

H + [NH4]+ → NH3 + H2
[PNH3]+ + e → P + NH3

Interstellar destruction mechanisms

[edit]

There are 113 total proposed reactions leading to the destruction of NH3. Of these, 39 were tabulated in extensive tables of the chemistry among C, N and O compounds.[185] A review of interstellar ammonia cites the following reactions as the principal dissociation mechanisms:[177]

with rate constants of 4.39×10−9[186] and 2.2×10−9,[187] respectively. The above equations (1, 2) run at a rate of 8.8×10−9 and 4.4×10−13, respectively. These calculations assumed the given rate constants and abundances of [NH3]/[H2] = 10−5, [[H3]+]/[H2] = 2×10−5, [HCO+]/[H2] = 2×10−9, and total densities of n = 105, typical of cold, dense, molecular clouds.[188] Clearly, between these two primary reactions, equation (1) is the dominant destruction reaction, with a rate ≈10,000 times faster than equation (2). This is due to the relatively high abundance of [H3]+.

Single antenna detections

[edit]

Radio observations of NH3 from the Effelsberg 100-m Radio Telescope reveal that the ammonia line is separated into two components–a background ridge and an unresolved core. The background corresponds well with the locations previously detected CO.[189] The 25 m Chilbolton telescope in England detected radio signatures of ammonia in H II regions, HNH2O masers, H–H objects, and other objects associated with star formation. A comparison of emission line widths indicates that turbulent or systematic velocities do not increase in the central cores of molecular clouds.[190]

Microwave radiation from ammonia was observed in several galactic objects including W3(OH), Orion A, W43, W51, and five sources in the galactic centre. The high detection rate indicates that this is a common molecule in the interstellar medium and that high-density regions are common in the galaxy.[191]

Interferometric studies

[edit]

VLA observations of NH3 in seven regions with high-velocity gaseous outflows revealed condensations of less than 0.1 pc in L1551, S140, and Cepheus A. Three individual condensations were detected in Cepheus A, one of them with a highly elongated shape. They may play an important role in creating the bipolar outflow in the region.[192]

Extragalactic ammonia was imaged using the VLA in IC 342. The hot gas has temperatures above 70 K, which was inferred from ammonia line ratios and appears to be closely associated with the innermost portions of the nuclear bar seen in CO.[193] NH3 was also monitored by VLA toward a sample of four galactic ultracompact HII regions: G9.62+0.19, G10.47+0.03, G29.96−0.02, and G31.41+0.31. Based upon temperature and density diagnostics, it is concluded that in general such clumps are probably the sites of massive star formation in an early evolutionary phase prior to the development of an ultracompact HII region.[194]

Infrared detections

[edit]

Absorption at 2.97 micrometres due to solid ammonia was recorded from interstellar grains in the Becklin–Neugebauer Object and probably in NGC 2264-IR as well. This detection helped explain the physical shape of previously poorly understood and related ice absorption lines.[195]

A spectrum of the disk of Jupiter was obtained from the Kuiper Airborne Observatory, covering the 100 to 300 cm−1 spectral range. Analysis of the spectrum provides information on global mean properties of ammonia gas and an ammonia ice haze.[196]

A total of 149 dark cloud positions were surveyed for evidence of 'dense cores' by using the (J,K) = (1,1) rotating inversion line of NH3. In general, the cores are not spherically shaped, with aspect ratios ranging from 1.1 to 4.4. It is also found that cores with stars have broader lines than cores without stars.[197]

Ammonia has been detected in the Draco Nebula and in one or possibly two molecular clouds, which are associated with the high-latitude galactic infrared cirrus. The finding is significant because they may represent the birthplaces for the Population I metallicity B-type stars in the galactic halo that could have been borne in the galactic disk.[198]

Observations of nearby dark clouds

[edit]

By balancing and stimulated emission with spontaneous emission, it is possible to construct a relation between excitation temperature and density. Moreover, since the transitional levels of ammonia can be approximated by a 2-level system at low temperatures, this calculation is fairly simple. This premise can be applied to dark clouds, regions suspected of having extremely low temperatures and possible sites for future star formation. Detections of ammonia in dark clouds show very narrow lines – indicative not only of low temperatures, but also of a low level of inner-cloud turbulence. Line ratio calculations provide a measurement of cloud temperature that is independent of previous CO observations. The ammonia observations were consistent with CO measurements of rotation temperatures of ≈10 K. With this, densities can be determined, and have been calculated to range between 104 and 105 cm−3 in dark clouds. Mapping of NH3 gives typical clouds sizes of 0.1 pc and masses near 1 solar mass. These cold, dense cores are the sites of future star formation.

UC HII regions

[edit]

Ultra-compact HII regions are among the best tracers of high-mass star formation. The dense material surrounding UCHII regions is likely primarily molecular. Since a complete study of massive star formation necessarily involves the cloud from which the star formed, ammonia is an invaluable tool in understanding this surrounding molecular material. Since this molecular material can be spatially resolved, it is possible to constrain the heating/ionising sources, temperatures, masses, and sizes of the regions. Doppler-shifted velocity components allow for the separation of distinct regions of molecular gas that can trace outflows and hot cores originating from forming stars.

Extragalactic detection

[edit]

Ammonia has been detected in external galaxies,[199][200] and by simultaneously measuring several lines, it is possible to directly measure the gas temperature in these galaxies. Line ratios imply that gas temperatures are warm (≈50 K), originating from dense clouds with sizes of tens of parsecs. This picture is consistent with the picture within our Milky Way galaxy – hot dense molecular cores form around newly forming stars embedded in larger clouds of molecular material on the scale of several hundred parsecs (giant molecular clouds; GMCs).

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Ammonia is a colorless with the NH₃, consisting of one atom bonded to three atoms in a trigonal pyramidal structure. It exists as a gas at , exhibiting a sharp, pungent detectable at concentrations as low as 5 parts per million, and is highly soluble in water where it partially dissociates to form ammonium hydroxide, a with pKa around 9.25. Ammonia ranks among the most produced chemicals globally, with annual output exceeding 180 million metric tons, primarily synthesized via the Haber-Bosch process that combines atmospheric with derived from under high pressure (150-300 atm) and temperature (400-500°C) using iron-based catalysts. In , approximately 80% of ammonia is converted into fertilizers such as and , enabling enhanced crop yields by supplying essential for growth and supporting global production for billions. Industrially, it serves as a precursor for explosives like TNT, refrigerants in large-scale cooling systems due to its high of , and agents leveraging its to dissolve grease and proteins. Despite these utilities, ammonia poses significant hazards as a corrosive irritant; of concentrations above 300 ppm can cause immediate danger to life and health, leading to , while skin contact results in severe burns, and it is acutely toxic with an LC50 of 2000 ppm for 1-hour rat exposure. Its production also contributes substantially to global CO₂ emissions, accounting for about 1-2% of anthropogenic greenhouse gases due to generation via reforming. Emerging research explores "green" ammonia via electrolysis-powered synthesis to mitigate these environmental impacts, though scalability remains limited.

Chemical and Physical Properties

Molecular Structure and Bonding

Ammonia has the molecular formula NH₃, consisting of a central atom bonded to three atoms via covalent bonds. The atom possesses five valence electrons, forming three N-H bonds and retaining a , which dictates its electronic structure. The bonding arises from the overlap of nitrogen's sp³ hybridized orbitals with the 1s orbitals of atoms, where the nitrogen's 2s and three 2p orbitals hybridize to form four equivalent sp³ orbitals directed towards the vertices of a . This hybridization accommodates the three bonding pairs and one . The of ammonia is trigonal pyramidal, as the occupies one sp³ orbital, causing repulsion that distorts the structure from tetrahedral. The H-N-H bond angle measures 107.8°, narrower than the ideal tetrahedral angle of 109.5° due to greater repulsion from the compared to bonding pairs. The N-H is 101.7 pm, reflecting the partial double-bond character absent in pure single bonds but influenced by differences. 's (3.04 on the Pauling scale) exceeds 's (2.20), rendering each N-H bond polar with partial negative charge on nitrogen and positive on hydrogen. The overall molecule is polar, with a dipole moment of 1.47 D directed from the hydrogen atoms toward the nitrogen lone pair, arising from the vector sum of individual bond dipoles and the lone pair's contribution. In molecular orbital terms, the valence orbitals form bonding, non-bonding, and antibonding combinations, with the highest occupied molecular orbital primarily localized on nitrogen's lone pair, explaining ammonia's basicity and nucleophilicity. Experimental data from sources like the NIST Computational Chemistry Comparison and Benchmark Database confirm these structural parameters through spectroscopic measurements.

Thermodynamic and Phase Properties

Ammonia's phase behavior is characterized by a at 195.4 K (−77.8 °C) and 6.06 kPa, where , , and vapor phases coexist in equilibrium. The normal at 1 atm is 195.0 K (−78.2 °C), with an of 331 kJ/kg (5.63 kJ/mol). The normal at 1 atm is 239.8 K (−33.3 °C), accompanied by a of of 1370 kJ/kg (23.4 kJ/mol). The critical point occurs at 405.4 K (132.2 °C) and 113 bar (11.3 MPa), beyond which distinct liquid and gas phases cannot be differentiated. Thermodynamic properties include heat capacities that vary by phase and temperature. For gaseous ammonia, the isobaric heat capacity (Cp) at 298 and ideal conditions is 35.6 J/mol·, increasing with temperature as described by the Shomate equation: Cp° = A + Bt + Ct² + Dt³ + E/t², with parameters fitted to experimental data yielding values such as 38.8 J/mol· at 400 . Liquid ammonia exhibits a of approximately 4.7 kJ/kg· near its , while solid ammonia's heat capacity follows Debye theory trends, measured at around 35 J/mol· near the .
PropertyValueConditions
Triple point temperature195.4 K6.06 kPa
Critical temperature405.4 K113 bar
Enthalpy of vaporization23.4 kJ/molAt 239.8 K
Gas Cp (298 K)35.6 J/mol·KIdeal gas

Chemical Reactivity and Solvent Behavior

Ammonia functions primarily as a Brønsted-Lowry base by accepting protons, forming ammonium ions: NH₃ + H⁺ → NH₄⁺, with reactions to strong acids being highly exothermic and potentially violent due to the strong N-H bond in the product. It also acts as a Lewis base, donating its nitrogen lone pair to electron-deficient species, as seen in adduct formation with boron trifluoride (NH₃·BF₃) or coordination to transition metals, exemplified by hexaamminecobalt(III) chloride ([Co(NH₃)₆]Cl₃). Ammonia reacts with halogens under controlled conditions to yield nitrogen halides like nitrogen trichloride (NCl₃), which is explosive, but excess ammonia produces ammonium halides; uncontrolled mixtures can lead to detonation. Oxidation of ammonia yields nitrogen gas or oxides depending on conditions: catalytic oxidation over platinum at 800–900°C produces nitric oxide (4NH₃ + 5O₂ → 4NO + 6H₂O), a key step in the Ostwald process for nitric acid production. Ammonia reduces with alkali metals to form metal amides, such as sodium amide (2Na + 2NH₃ → 2NaNH₂ + H₂), and ignites spontaneously with strong oxidizers like chlorine or bromine. In combustion, it burns in oxygen to nitrogen and water (4NH₃ + 3O₂ → 2N₂ + 6H₂O), though incomplete combustion risks NOx formation. Liquid ammonia, boiling at −33.34°C under standard pressure, behaves as a polar aprotic-like solvent with a dielectric constant of 22 at −35°C, promoting ionization of salts more effectively than expected from its value alone due to hydrogen bonding networks similar to but weaker than water's. It autoionizes minimally: 2NH₃ ⇌ NH₄⁺ + NH₂⁻, with an equilibrium constant K ≈ 10⁻³³ at −50°C, far lower than water's Kw = 10⁻¹⁴ at 25°C, resulting in poor conductivity but enabling amphoteric behavior where it levels strong acids to NH₄⁺ and strong bases to NH₂⁻. This solvent dissolves alkali metals to yield intensely colored solutions of solvated electrons (e.g., Na in NH₃(l) gives a blue bronze hue), providing powerful reducing conditions for reactions like the of aromatic compounds. Liquid ammonia excels at solubilizing nonpolar organics and certain halides poorly soluble in , facilitating syntheses such as alkali metal-mediated deprotonations or substitutions unattainable in protic media.

Spectroscopic and Analytical Characteristics

Ammonia exhibits four fundamental vibrational modes arising from its pyramidal C_{3v} : the symmetric N-H stretch (ν_1, a_1), degenerate asymmetric N-H stretches (ν_3, e), degenerate H-N-H bends (ν_2, e), and umbrella inversion (ν_4, a_1). In the gas phase, the symmetric stretch appears at approximately 3337 cm⁻¹, primarily Raman active, while the asymmetric stretches occur at 3444 cm⁻¹, active. The bending mode is observed near 1627 cm⁻¹ in the spectrum, and the inversion mode around 968 cm⁻¹, active in both and Raman. These frequencies shift in condensed phases or clusters due to hydrogen bonding, with broader, lower-energy bands in aqueous solutions. The rotational microwave spectrum of ammonia is distinguished by inversion doubling from quantum tunneling through the pyramidal barrier, splitting each rotational level into symmetric and antisymmetric states. The most prominent transition, for the J=3, K=3 level in the ground vibrational state, occurs at 23.787 GHz, enabling precise frequency standards and early applications. Higher J and K transitions extend up to tens of GHz, with linewidths influenced by pressure broadening and dipole moment effects. In , the ¹H spectrum of ammonia features a broad near 1 ppm (relative to TMS) due to quadrupolar relaxation from ¹⁴N (I=1), resulting in no resolved and short T₂ times. ¹⁵N-labeled ammonia (I=1/2) yields sharp ¹H-¹⁵N doublets with J ≈ 60 Hz, facilitating quantification in aqueous media, though paramagnetic additives like Gd³⁺ can accelerate relaxation for faster acquisition. ¹⁴N NMR shows a single peak but is broadened similarly, with chemical shifts around 0 ppm in . Ultraviolet absorption of ammonia is weak above 200 nm, with structured bands from the ùA₂ ← X̃¹A₁ transition between 190-230 nm, cross-sections increasing with due to hot bands. Stronger continuous absorption begins below 1665 Å, transitioning to diffuse Rydberg series toward 1200 Å. In , the base peak is the molecular ion NH₃⁺ at m/z 17 (100% relative intensity), with minor fragments including NH₂⁺ (m/z 16, ~1-5%) and trace H₃⁺ (m/z 3) from dissociative ionization; fragmentation is limited due to the molecule's stability. Spectroscopic methods serve as key analytical tools for ammonia detection and quantification. identifies gas-phase NH₃ via N-H stretches and enables trace-level monitoring in ambient air. detects aqueous ammonia at low concentrations (ppm) using fingerprint vibrations around 934-967 cm⁻¹. UV spectroscopy quantifies via absorption cross-sections in the 190-230 nm range, suitable for high-temperature or process monitoring. These techniques offer specificity over colorimetric alternatives, though interferences from water or CO₂ require matrix isolation or derivatization in complex samples.

Natural Occurrence and Detection

Abiotic Sources

Abiotic sources of ammonia on primarily arise from geological processes, including volcanic and hydrothermal activities, though their contributions to global ammonia budgets are minor compared to biotic emissions. Volcanic emissions, such as those from fumarolic vents, release ammonia gas directly into the atmosphere, with global estimates indicating approximately 0.9 teragrams of per year (TgN yr⁻¹) from volcanic sources. observations have confirmed elevated ammonia concentrations coinciding with thermal hotspots at fumaroles, as documented in Nicaraguan volcanic systems where fault-line emissions produce detectable plumes. In hydrothermal systems, abiotic reduction of (NO₃⁻) and (NO₂⁻) to (NH₄⁺) occurs under reducing conditions during high-temperature fluid circulation, particularly in subseafloor environments. Iron-bearing minerals, such as mackinawite (FeS), facilitate this process by enhancing ammonia adsorption and reduction, potentially accumulating significant NH₃ in vent fluids. Experimental simulations of hydrothermal conditions demonstrate stable abiotic from , with reaction kinetics favoring NH₄⁺ as the dominant product (>50% yield) alongside nitrogen gas. Estimated production rates in such systems range from 10⁵ to 10¹⁰ moles per year, depending on availability in , though these fluxes remain geochemically limited. Atmospheric processes like do not significantly produce ammonia naturally; while mimics using plasma discharges generate NH₃ from N₂ and H₂O, natural primarily fixes as rather than NH₃. On , mineral-catalyzed reduction of N₂ by Fe-Ni metals or shock synthesis involving iron and water may have supplied ammonia to primordial oceans, but contemporary abiotic fluxes from these mechanisms are negligible. Overall, these abiotic pathways underscore ammonia's geochemical cycling independent of , yet empirical data indicate they constitute a small of modern environmental ammonia, overshadowed by anthropogenic and biotic inputs.

Biotic Production

Biological nitrogen fixation by prokaryotic organisms constitutes the principal biotic pathway for ammonia synthesis from atmospheric dinitrogen (N₂), enabling the incorporation of inert into bioavailable forms essential for . Diazotrophic bacteria (e.g., , ) and employ the metalloenzyme , which catalyzes the ATP-dependent reduction of N₂ to ammonia (NH₃) via the reaction N₂ + 8H⁺ + 8e⁻ + 16ATP → 2NH₃ + + 16ADP + 16Pᵢ, with a stoichiometric byproduct of gas. This process demands anaerobic conditions or protective mechanisms, as nitrogenase is oxygen-sensitive, and occurs in diverse ecological niches: symbiotic mutualisms (e.g., in root nodules exchanging NH₃ for plant carbohydrates), associative symbioses with grasses, and free-living soil or aquatic microbes. Globally, biological contributes an estimated 100–200 teragrams of annually, rivaling pre-industrial inputs before synthetic fertilizers dominated. Ammonification, or mineralization, represents another key biotic source, wherein heterotrophic bacteria and fungi decompose nitrogenous organic matter—such as proteins, amino acids, nucleic acids, and —releasing inorganic ammonia or (NH₄⁺). This excretory process is mediated by saprotrophs including , , , , and species, which hydrolyze organic N via proteases, ureases, and deaminases, yielding NH₃ that equilibrates with NH₄⁺ depending on and conditions. In terrestrial ecosystems, ammonification recycles from decaying and animal wastes, while in aquatic environments, it supplements fixation by processing phytoplankton detritus and zooplankton excretion. Unlike fixation, ammonification does not introduce new but mobilizes existing pools, with rates influenced by , , and carbon availability; for instance, optimal activity occurs at 25–35°C in aerated soils. Animal metabolism also generates ammonia transiently through , where and oxidative produce NH₃ as a nitrogenous waste, though terrestrial vertebrates primarily convert it to less toxic or via the ornithine-urea cycle to minimize . Aquatic and , however, excrete ammonia directly into , contributing localized biotic fluxes in freshwater and marine systems—e.g., up to 80–90% of nitrogen by occurs as NH₃ under favorable dilution conditions. These processes underscore ammonia's role as a labile intermediate in biotic nitrogen dynamics, prone to rapid uptake by plants or oxidation by nitrifiers, thereby sustaining productivity without net atmospheric drawdown beyond fixation.

Detection and Measurement Techniques

Ammonia concentrations in environmental, industrial, and biological matrices are quantified using a variety of analytical techniques, selected based on the sample type, required sensitivity, and detection range. Colorimetric methods predominate for aqueous samples, leveraging chemical reactions to produce measurable color changes. The , standardized in EPA Method 350.1, involves reacting ammonia with alkaline phenol and to form a , followed by spectrophotometric measurement at approximately 630 nm, enabling detection down to 0.02 mg/L in drinking, surface, and wastewater. Nessler's reagent, a mercuric-potassium solution, forms a yellow-brown colloidal complex with ammonia, detectable at 400-425 nm, though it requires careful handling due to mercury and interference from . Electrochemical methods, including ion-selective electrodes (ISEs), offer real-time, portable detection for ammonia in and extracts. Ammonia ISEs measure the potential difference generated by NH₄⁺ ions after adjustment to liberate free NH₃, with linear response typically from 0.03 to several thousand mg/L, though calibration with ionic strength adjusters is essential to mitigate matrix effects. For , ammonia is extracted using solutions before analysis, ensuring total nitrogen recovery. Gaseous ammonia in air is monitored via and -based techniques. Fourier-transform (FTIR) quantifies NH₃ by absorption at 10.3-10.8 μm, suitable for stack emissions and ambient monitoring with detection limits around 1 ppm. Photoacoustic enhances sensitivity to parts-per-billion levels by detecting acoustic waves from absorbed laser energy. Passive denuders, coated with absorbing acids, capture NH₃ for subsequent analysis, providing time-integrated measurements in agricultural and atmospheric studies with low detection limits of 0.1 μg/m³. Active sampling with acid bubblers or detectors measures higher concentrations in industrial settings. Advanced instrumental methods like (GC) coupled with thermal conductivity or detect ammonia in complex mixtures, such as bioreactor headspaces, following derivatization to improve volatility, with quantification limits below 1 ppm. (SERS) enables rapid, low-concentration aqueous detection via vibrational fingerprints enhanced by nanostructured substrates. separates and quantifies ions in water and extracts using conductivity detection after suppression, ideal for trace levels in pharmaceuticals and soils. These techniques collectively ensure accurate monitoring, with method selection guided by factors like interference susceptibility and regulatory requirements.

Industrial Production

Haber-Bosch Process

The Haber-Bosch process synthesizes from and gases via the reversible reaction N₂ + 3H₂ ⇌ 2NH₃, which is exothermic with a standard change of -92 kJ/mol. German chemist first demonstrated the reaction on a scale in 1909, achieving synthesis under high pressure and temperature with an iron catalyst. , working at , engineered the industrial-scale version, with the first commercial plant operational at Oppau, , in 1913, producing 30 tonnes of per day initially. The process operates at 400–450 °C and 15–25 MPa (150–250 bar) using a promoted iron catalyst, typically containing and alumina to enhance activity and suppress reverse reaction effects. These conditions balance and kinetics: high pressure shifts the equilibrium toward ammonia per , while elevated temperature accelerates the rate-limiting nitrogen dissociation on the catalyst surface despite favoring the endothermic reverse reaction. Unreacted gases are recycled after condensation of ammonia at lower temperatures, yielding overall efficiencies of 90–95% despite single-pass conversions of 10–20%. Hydrogen feedstock derives primarily from of (CH₄ + H₂O → CO + 3H₂, followed by water-gas shift: CO + H₂O → CO₂ + H₂), accounting for 70% of the process's energy input, with separated from air via cryogenic . Globally, the process accounts for over 90% of , totaling around 180 million metric tonnes annually as of recent estimates, but consumes 1–2% of world energy and 3–5% of supplies. This synthesis enabled mass production of nitrogen fertilizers, underpinning the Green Revolution's tripling of global crop yields since 1950, though its dependence contributes about 1% of anthropogenic CO₂ emissions. Ongoing optimizations focus on improvements and process integration to reduce , currently around 28–35 GJ per of ammonia.

Alternative Synthesis Methods

Electrochemical methods for ammonia synthesis involve the direct reduction of gas using , typically under ambient conditions, as an alternative to the high-temperature, high-pressure requirements of the Haber-Bosch process. These approaches couple renewable sources, such as solar or , to drive the reaction N₂ + 6H⁺ + 6e⁻ → 2NH₃, often in aqueous or non-aqueous electrolytes with catalysts like transition metals or single-atom sites. Despite theoretical appeal for decentralized production, yields remain low, with Faradaic efficiencies for N₂ reduction typically below 10-20% in most systems due to competing hydrogen evolution and poor N₂ activation. Variants include lithium-mediated cycling, where molten reduces N₂ in aprotic solvents, achieving rates up to 10⁻⁵ mol NH₃ m⁻² s⁻¹ but requiring energy inputs comparable to or exceeding Haber-Bosch when scaled. reduction pathways, using as feedstock, have reported higher efficiencies—up to 75% Faradaic efficiency on Fe single-atom catalysts—but these bypass direct N₂ fixation and depend on pre-existing nitrogen oxides. Plasma-assisted catalysis represents another pathway, leveraging non-thermal plasma to generate like N radicals or vibrationally excited N₂, which overcome kinetic barriers at temperatures below 300°C. In these systems, barrier discharges or gliding arc plasmas are combined with catalysts such as Ru or Fe on supports, enabling ammonia yields beyond limits—e.g., single-pass conversions of 5-10% at . The process integrates well with intermittent renewables for small-scale, modular plants, with energy efficiencies reported at 10-15% for NH₃ production from N₂ and H₂, though scaling challenges include electrode and . Recent innovations, such as water-mediated plasma reactors, aim to eliminate separate H₂ by direct N₂-H₂O , yielding up to 0.1 g kWh⁻¹ NH₃ in lab tests. Biological routes, drawing from nitrogenase enzymes in microbes like Azotobacter or engineered yeasts, offer a low-energy fixation mechanism but face scalability hurdles for industrial output. These processes convert N₂ to NH₃ using ATP-driven enzymes under ambient conditions, with lab demonstrations achieving 10-100 mg/L yields from feedstocks like soy meal via hyper-ammonia-producing . However, enzyme instability and oxygen sensitivity limit continuous operation, rendering them unsuitable for large-scale replacement of Haber-Bosch, which produces over 180 million tonnes annually. Hybrid bio-electrochemical systems are under exploration to boost rates, but commercial viability remains distant. Other niche methods, such as mechanochemical synthesis via high-speed ball milling of N₂, H₂, and Fe catalysts, have produced continuous NH₃ streams at room temperature in pilot setups, with yields of ~0.02 g h⁻¹ g_cat⁻¹, but energy demands from mechanical input rival traditional processes. Overall, while these alternatives promise reduced carbon footprints when paired with green hydrogen, none have achieved cost-competitive, gigatonne-scale production as of 2025, constrained by catalyst selectivity and overpotential losses.

Global Production and Economic Scale

Global ammonia production exceeded 190 million metric tons in 2024, with estimates ranging from 191 million tons in 2023 to 194.8 million tons the following year, primarily driven by demand for fertilizers. The Haber-Bosch process dominates, accounting for over 90% of output, concentrated in regions with access to low-cost or feedstocks. China leads as the largest producer, contributing about 30% of global supply, followed by the , , , and the , where production aligns with agricultural needs and energy availability. Production capacity worldwide stood at approximately 240 million tons as of recent assessments, with expansions projected to add 6% over the next four years, particularly in low-cost regions like the and . Export volumes highlight trade dynamics, with , , and as top anhydrous ammonia exporters in 2023, shipping millions of tons to import-dependent agricultural economies. These figures underscore ammonia's role as a bulk , with over 80% directed toward nitrogenous fertilizers, sustaining global food production amid . Economically, ammonia production consumes around 2% of global final energy (8.6 exajoules annually), reflecting its capital-intensive nature and reliance on fossil fuels for hydrogen generation. Market valuations vary by scope but indicate a sector worth $70-224 billion in 2024, influenced by volatile natural gas prices and fertilizer demand fluctuations. Projections forecast steady growth at 4-6% CAGR through 2030-2035, reaching 190-200 million tons annually, bolstered by emerging applications in clean energy carriers, though conventional "gray" ammonia will persist due to cost advantages over nascent green alternatives. This scale positions ammonia as a cornerstone of industrial chemistry, with production economics tightly linked to energy markets and agricultural output.

Applications

Fertilizers and Agricultural Impact

Approximately 80% of the world's is directed toward applications, primarily in the form of ammonia for direct injection or as a precursor to compounds like , , and . Global ammonia output reached about 191 million metric tons in 2023, with 170–180 million metric tons allocated to agricultural uses, underscoring 's role as a limiting in growth. These fertilizers supply essential for protein synthesis in , enhancing , leaf expansion, and overall accumulation. The Haber-Bosch process, enabling scalable ammonia synthesis since its industrialization in the , triggered a transformation in akin to a . Synthetic fertilizers have boosted global yields by factors of 2–3 in staple grains like , , and compared to pre-1900 levels reliant on natural sources such as and . Without this process, analyses estimate that Earth's for food production would support only about half the current population of 8 billion, as natural cycles limit soil replenishment. In the U.S., corn yields rose from under 30 bushels per acre in to over 175 bushels per acre by , with applications accounting for 40–50% of yield gains alongside hybrid seeds and . Agriculturally, ammonia-derived fertilizers have reduced risks and enabled arable expansion on marginal , but inefficiencies persist: only 50–70% of applied is typically crop-absorbed, with losses via volatilization or leaching necessitating precise application timing and rates to avoid yield plateaus or nutrient imbalances. Over-application, observed in intensive systems, can acidify (lowering by 0.2–0.5 units over decades) and disrupt microbial communities essential for , though banded or fertigated delivery mitigates these effects. tools, integrating testing and variable-rate technology, have improved use efficiency to 60–80% in optimized fields, sustaining long-term productivity without proportional input increases.

Chemical Synthesis Precursors

Ammonia serves as a primary feedstock for nitric acid production via the Ostwald process, where it is catalytically oxidized with oxygen over a platinum-rhodium gauze catalyst at approximately 900°C to form nitric oxide, which is further oxidized to nitrogen dioxide and absorbed in water to yield nitric acid with near-complete conversion efficiency. This nitric acid is then used to synthesize intermediates such as adipic acid for nylon-6,6 and hydroxylamine for caprolactam in nylon-6 production, as well as nitroaromatics and other compounds for dyes, pharmaceuticals, and explosives precursors like ammonium nitrate formed by neutralizing nitric acid with additional ammonia. In the Sohio ammoxidation process, ammonia reacts with and air in a fluidized-bed reactor over a bismuth-molybdenum at 400-500°C, producing with selectivities exceeding 80%, which serves as a building block for ABS plastics, acrylic fibers, , and for in nylon-6,6 synthesis. This one-step vapor-phase method, commercialized in the , revolutionized production by replacing older, multi-step routes and now accounts for over 90% of global output, derived from roughly 5-10% of industrial ammonia consumption. Ammonia is also alkylated with alcohols or olefins under acidic or dehydrating conditions to generate aliphatic , such as methylamines from and ammonia at 300-400°C over alumina catalysts, yielding mixtures used in , agrochemicals, solvents, and pharmaceutical intermediates like ephedrine precursors. These processes, often unreacted ammonia, enable high-purity production essential for downstream and manufacturing, with global amine capacity tied to ammonia availability exceeding millions of tonnes annually. Additional syntheses include from ammonia and via the Raschig process, used in rocket fuels and pharmaceuticals, and from ammonia and under high pressure for resins in adhesives and coatings, though the latter represents a minor fraction of ammonia use compared to nitric acid and routes. Overall, these applications consume about 20-30% of produced ammonia, underscoring its role in nitrogen-containing and specialty chemical chains.

Refrigeration and Industrial Processes

Ammonia serves as a primary in large-scale industrial cooling systems due to its thermodynamic efficiency and environmental profile. First applied in during the 1850s and in the United States in the 1860s for artificial ice production, it enabled the expansion of during the . Its adoption persisted through improvements in technology in the 1930s and 1940s, refining purity to nearly 100% for and gas applications. Key properties include a high of , allowing substantial heat absorption per unit mass, which contributes to 3-10% greater compared to chlorofluorocarbons (CFCs) and hydrochlorofluorocarbons (HCFCs). Ammonia exhibits zero (ODP) and zero (GWP), positioning it as a natural alternative amid phase-outs of synthetic refrigerants under international agreements like the . Refrigerant-grade ammonia is colorless, odorless in pure form, and at least 99.95% pure, though detectable by its pungent smell at concentrations above 5 parts per million. Industrial applications dominate, with ammonia comprising 80-90% of U.S. industrial capacity, particularly in , cold storage warehouses, breweries, and chemical plants requiring temperatures below -30°C. Globally, it remains the most common for large commercial systems, though only approximately 2% of annual —around 2 million metric tons out of 100 million—is allocated to refrigeration. indicate the ammonia refrigerants sector valued at USD 55.5 million in 2022, projected to reach USD 86.5 million by 2030 at a 5.7% , driven by demand for low-GWP solutions. Broader industrial refrigeration systems incorporating ammonia reached USD 9.7 billion in 2024. Safety protocols mitigate risks from ammonia's toxicity and flammability in concentrations above 16% by volume in air. Systems operate under stringent U.S. (OSHA) guidelines, including and ventilation, rendering incidents attributable largely to failures rather than inherent instability. In absorption refrigeration processes, ammonia pairs with as an absorbent for and recovery, enhancing energy efficiency in cogeneration plants. Despite these advantages, regulatory scrutiny persists due to potential exposure hazards, necessitating like double-walled and remote monitoring.

Fuel and Energy Applications

Ammonia serves as a carbon-free and carrier in applications, leveraging its ability to store and at moderate pressures and temperatures compared to pure . Produced via the Haber-Bosch process using renewable for electrolysis-derived —termed "green ammonia"—it enables long-distance shipping without cryogenic requirements, with a volumetric of approximately 108 g/L at -33°C and 1 bar, higher than liquid 's 70 g/L. This positions ammonia for roles in maritime and power , where for its handling already exists from trade. In combustion systems, ammonia's lower heating value of 18.6 MJ/kg—about 40% that of diesel—necessitates engine modifications such as higher compression ratios, pilot fuels like hydrogen or methane for ignition, and NOx mitigation via selective catalytic reduction due to nitrogen content yielding up to 100% NOx in unmitigated burns. Gas turbine demonstrations, including Mitsubishi Heavy Industries' tests achieving stable combustion with 100% ammonia blends, target stationary power plants for grid balancing with renewables. Internal combustion engines, such as a prototype 2-liter ammonia-fueled unit developed in 2025, operate via direct injection and spark ignition, delivering zero-carbon output but requiring additives to address slow flame speeds. Fuel cell technologies convert ammonia indirectly to electricity, often via cracking to hydrogen followed by proton exchange membrane or solid oxide cells, bypassing combustion emissions. Amogy's ammonia-to-power system, deploying non-combustion reformers, powers stationary and mobile units with efficiencies up to 60%, as validated in 2025 pilots for heavy-duty transport. In shipping, ammonia fuels dual-fuel engines and fuel cells, with the NEOM Green Hydrogen Complex in Saudi Arabia producing 600 tonnes per day of green ammonia since 2023 for export as maritime fuel. Regulatory advancements, including bunkering pilots in Norway and Singapore, signal commercialization, though high production costs—around $350–600 per tonne for green variants—limit scalability without subsidies. The global fuel ammonia market reached $1.7 billion in 2025, driven by shipping decarbonization targets under IMO regulations aiming for net-zero by 2050, yet adoption hinges on resolving toxicity risks during handling and ensuring supply chains from renewable sources to avoid reliance on fossil-derived "" ammonia. Empirical tests confirm feasibility in controlled environments, but full-scale deployment requires empirical validation beyond lab-scale, as current applications remain pilot-stage with no widespread grid or fleet integration as of October 2025.

Other Specialized Uses

Ammonia solutions, typically 5–10% aqueous , are employed as effective agents in both household and industrial applications, leveraging their alkaline properties to emulsify oils, dissolve mineral deposits, and remove protein-based stains from surfaces such as , , and metals. In industrial cleaning, or concentrated ammonia is used for equipment in and facilities, where it provides rapid evaporation without residue. In processes, ammonia is applied as a chloramine precursor by reacting with to form , a stable that maintains residual activity in distribution systems, reducing bacterial regrowth compared to free alone; this method has been standard in U.S. municipal supplies since the early , with facilities dosing 1–5 mg/L of ammonia. Ammonia also aids in adjustment and odor control in , where it neutralizes acidic effluents and precipitates . The textile industry utilizes ammonia for fabric processing, including scouring to remove impurities from wool and cotton, dyeing as a mordant to fix colors, and treating fibers to enhance shrinkage resistance and durability; for instance, aqueous ammonia solutions are applied in the production of rayon and in mercerization alternatives for cotton. In synthetic fiber manufacturing, ammonia facilitates polymerization steps for materials like nylon, though its role is ancillary to primary synthesis. Ammonia serves as a critical precursor in the manufacture of explosives, particularly , which is produced by neutralizing with ammonia gas and crystallized for use in , quarrying, and ; global production of ammonium nitrate explosives exceeds 20 million metric tons annually, with ammonia comprising about 80% of its nitrogen content by weight. In metallurgy, ammonia is used in processes to introduce into surfaces, forming hard layers that improve wear resistance and fatigue strength; this thermochemical treatment, developed in the , operates at 500–570°C and is applied to components like gears and crankshafts in automotive and industries.

Environmental and Health Considerations

Toxicity and Human Health Effects

Ammonia exerts its primary toxic effects through direct irritation and corrosion of moist tissues, particularly in the , eyes, and , due to its alkaline nature and ability to react with to form ammonium hydroxide. is the most common route of exposure in occupational and accidental settings, with concentrations exceeding 30 ppm causing immediate irritation to the nose, throat, and upper . At higher levels, such as 100-200 ppm, symptoms progress to coughing, choking, and chest tightness, while exposures above 500 ppm can induce severe respiratory distress, , and potentially fatal laryngeal spasm or asphyxiation. The immediately dangerous to life or health (IDLH) concentration is 300 ppm, beyond which escape without assistance may be impossible. Ocular exposure to ammonia vapor or liquid results in rapid corneal ulceration and potential blindness, with even brief contact at concentrations over 100 ppm causing lacrimation, , and conjunctival . Dermal contact with anhydrous ammonia leads to liquefaction and due to its low (-33°C), manifesting as severe burns, blisters, and tissue destruction; diluted solutions (e.g., 5-10% in cleaners) cause less severe but still painful . , though rare, produces immediate burning in the , , and , potentially leading to , , and . Occupational exposure limits reflect these hazards:
AgencyLimit TypeValue
OSHAPEL (8-hour )50 ppm (35 mg/m³)
NIOSHREL (10-hour )25 ppm (18 mg/m³)
NIOSHREL (15-min STEL)35 ppm (27 mg/m³)
ACGIHTLV (8-hour )25 ppm
Chronic low-level exposure may sensitize airways, increasing susceptibility to asthma-like symptoms or , though systemic toxicity is limited as ammonia is rapidly neutralized in the body unless overwhelming. Treatment involves immediate removal from exposure, decontamination with (avoiding neutralization to prevent exothermic reactions), supportive care for respiration, and ophthalmologic intervention for eyes; no specific exists.

Ecological Impacts and Pollution

Ammonia emissions, predominantly from agricultural sources comprising 81% of global totals, contribute significantly to environmental pollution through atmospheric deposition, runoff into water bodies, and direct releases. These emissions have risen by 78% between 1980 and 2018, driven by increased fertilizer use and livestock production, exacerbating ecological disruptions worldwide. In aquatic ecosystems, un-ionized ammonia (NH₃) exerts on and , damaging gills, inducing stress, and impairing at concentrations as low as 0.02 mg/L for sensitive species like salmonids, with toxicity intensifying at higher pH and temperatures due to the equilibrium shift favoring the more permeable NH₃ form over ammonium (NH₄⁺). Chronic exposure leads to reduced growth, , and heightened disease susceptibility, while acute levels exceeding 1-2 mg/L total ammonia can cause mass mortalities in freshwater and marine habitats. Ammonia also fuels by providing excess , promoting algal blooms that deplete oxygen and create hypoxic dead zones, as observed in nutrient-enriched rivers and coastal areas. Atmospheric ammonia undergoes rapid deposition within 4-5 km of sources, causing direct foliar injury to vegetation and lichens, , and enrichment that alters communities by favoring nitrophilous over oligotrophic ones, thereby reducing in grasslands, forests, and heathlands. Deposited ammonia forms ammonium salts contributing to secondary particulate matter (PM₂.₅) formation, which indirectly harms ecosystems via reduced visibility, altered precipitation chemistry, and enhanced effects. In terrestrial settings, excess from ammonia deposition disrupts microbial communities and intensifies in freshwater systems through hydrological linkages.

Debates on Sustainable Production Variants

The dominant Haber-Bosch process for ammonia synthesis, reliant on steam methane reforming of for , accounts for approximately 1-2% of global and emits around 1% of anthropogenic CO2, prompting debates over transitioning to lower-emission variants like blue ammonia (with ) and green ammonia (using electrolytic from renewables). Proponents of green ammonia argue it enables near-zero direct emissions by pairing water electrolysis powered by solar or wind with , potentially aligning with net-zero goals, but critics highlight that lifecycle assessments often reveal higher total energy demands due to electrolysis inefficiencies (typically 60-70% round-trip) and the need for overbuilding renewables to compensate for intermittency. Economic feasibility remains a core contention, with grey ammonia production costs averaging $300-500 per metric ton in 2023-2024, contrasted against green ammonia estimates of $600-1,000+ per ton, heavily dependent on electricity prices below $30/MWh for competitiveness—levels achievable only in optimal renewable sites but rare globally. Blue ammonia, capturing 90-95% of CO2 via CCS, offers a transitional path with costs 20-50% above under current carbon pricing, yet real-world CCS deployment has averaged capture rates below 85% in operational plants, raising doubts about its scalability and permanence given storage leakage risks over centuries. Studies indicate that without subsidies or carbon taxes exceeding $100/ CO2, variants retain advantages in regions with abundant , such as the or , where green pathways face grid and infrastructure bottlenecks. Scalability debates center on resource constraints: producing the global 180 million tons of ammonia annually via green methods would require electrolyzer capacity equivalent to 10-20% of projected 2050 renewable electricity, diverting power from electrification sectors where efficiency gains are higher, per thermodynamic analyses showing ammonia's end-use losses in fertilizers or fuels exceed direct alternatives. Emerging non-Haber-Bosch routes, like plasma-activated synthesis, promise lower energy inputs (under 10 GJ/ton vs. 28 GJ/ton for conventional), but remain lab-scale with unproven durability and yields below 1% as of 2025. Critics, including energy economists, contend that policy-driven mandates for green ammonia overlook causal trade-offs, such as increased land use for renewables (potentially 1-2% of arable land globally if scaled) and mineral demands for electrolyzers, exacerbating supply chain vulnerabilities without empirically demonstrated emissions reductions at gigaton scale. Food security implications fuel further contention, as ammonia-derived fertilizers underpin 50% of global crop yields; elevating costs through unsubsidized green production could disproportionately burden developing nations, where grey ammonia enables yields supporting 4 billion people, per agricultural impact models. While advocates cite pilot projects—like Australia's 2025 electrochemical breakthroughs using air and —yielding ammonia at lab efficiencies, skeptics note these ignore integration challenges, such as hydrogen storage volatility and activation barriers persisting below 400°C without high pressures. Overall, empirical data underscores that sustainable variants' viability hinges on technological leaps in catalysts and storage, yet as of 2025, no pathway matches grey ammonia's proven reliability for baseline demand.

Historical Development

Early Discovery and Uses

Ammonia compounds, particularly sal ammoniac (), were recognized in antiquity, with deposits collected near the Temple of Zeus Ammon in the of , derived from the evaporation of camel urine and dung. Ancient Egyptians, , and Romans utilized sal ammoniac as a for metals, in textiles, and for medicinal purposes such as treating digestive ailments and as an expectorant. These applications stemmed from its volatile properties when heated, releasing pungent vapors, though the compound's chemical nature remained unidentified until the . Gaseous ammonia was first isolated in the 1770s by English chemist , who obtained it by heating a mixture of sal ammoniac and quicklime () over mercury, collecting the "alkaline air" and noting its distinctive odor and solubility in water. Priestley described the gas's ability to extinguish flames and its reaction with acids to form salts, contributing to early understandings of pneumatic chemistry. In 1785, French chemist determined its composition as a compound of and , solidifying its identification as NH₃. Prior to industrial synthesis, ammonia was produced in small quantities by distilling animal horns, hooves, or —known as "spirit of hartshorn"—and employed as to revive the fainted by stimulating respiration through its irritating vapor. It served as a for its properties on grease and stains, and in leather processing for tanning hides by neutralizing acids. Limited fertilizer applications emerged in the 19th century from byproduct recovery in , where ammonia was scrubbed from , but natural sources like dominated agricultural supply until synthetic methods scaled up.

Haber-Bosch Industrialization

The Haber-Bosch process, developed by German chemist Fritz Haber, achieved laboratory-scale synthesis of ammonia from atmospheric nitrogen and hydrogen in 1909, building on earlier thermodynamic studies of the reversible reaction N₂ + 3H₂ ⇌ 2NH₃. Haber patented the method, which required high pressures to shift the equilibrium toward ammonia formation, addressing the scarcity of fixed nitrogen sources like guano and Chilean saltpeter that had previously limited agricultural output. Carl Bosch, leading a team at BASF, industrialized the process by solving engineering challenges, including the fabrication of high-pressure reactors from novel steel alloys to withstand 200-300 bar and temperatures of 400-530°C, where an iron catalyst promoted with alkali metals and alumina facilitates the reaction at rates sufficient for commercial viability. The first full-scale plant opened in Oppau, Germany, in , initially producing 20 tons of ammonia per day and scaling to 40 tons within a year through iterative optimizations in gas compression, catalyst durability, and recycle loops to handle the low single-pass conversion yields of 10-20%. This marked the first industrial application of high-pressure catalysis, supplanting energy-intensive alternatives like the arc process. The process's efficiency, though demanding 30-40 GJ per ton of ammonia due to compression and heating needs, enabled synthetic nitrogen fertilizers on a massive scale, with global capacity reaching millions of tons annually by the via subsequent plants like Leuna in 1917. By providing a reliable source independent of natural deposits, it catalyzed surges, supporting yields that sustained human from 1.6 billion in 1900 to over 6 billion by 2000, as via this method accounts for roughly half of the production underlying modern demographics. During , it also supplied for explosives, underscoring its dual role in enabling both sustenance and conflict.

Post-War Expansion and Innovations

Following World War II, ammonia production underwent massive expansion as wartime facilities, originally built for explosives, were repurposed for agricultural fertilizers to support global food security amid population growth. In the United States, government investments during the war positioned the country as the global leader in synthetic ammonia capacity by 1945, with production shifting rapidly from munitions to civilian uses; by the 1950s, U.S. output accounted for a significant portion of worldwide growth, driven by demand for nitrogen fertilizers. Globally, annual synthesis grew from under 300,000 metric tons in the late 1930s to millions of tons by the 1960s, fueled by the Haber-Bosch process's scalability and the need to boost crop yields; between 1950 and 1980, capacity expanded rapidly to meet surging fertilizer needs, enabling the Green Revolution's high-yield agriculture. Key innovations enhanced efficiency and reduced costs, including the widespread adoption of as a hydrogen feedstock via steam methane reforming, which replaced costlier or heavy oil partial oxidation methods prevalent before the 1950s; this shift, enabled by abundant low-cost , lowered energy inputs and impurities, allowing for larger-scale operations. designs evolved from multi-train, multi-pressure configurations to single-train, single-pressure systems with centrifugal compressors substituting reciprocating ones, improving reliability and throughput; quench converters, first installed in , became standard post-war, optimizing heat management in synthesis loops. Catalyst advancements further drove progress, with refined iron-based promoters increasing conversion rates and longevity under high-pressure conditions, contributing to energy savings of up to 30% in modernized by the compared to early Haber-Bosch setups. These developments not only scaled production to over 100 million metric tons annually by the late but also underscored the process's reliance on fossil fuels, prompting later scrutiny of its environmental footprint despite enabling unprecedented agricultural output.

Biological and Medical Roles

Biosynthesis Pathways

In biological systems, ammonia (NH₃) is primarily synthesized through , a process carried out by prokaryotes such as diazotrophic and , which convert atmospheric dinitrogen (N₂) into bioavailable ammonia via the enzyme . This reaction requires significant energy input, typically 16 ATP molecules per N₂ molecule reduced, and proceeds via the N₂ + 8H⁺ + 8e⁻ → 2NH₃ + H₂, with the byproduct gas representing an inefficiency of the pathway. consists of two key components: the iron protein (NifH), which transfers electrons, and the molybdenum-iron protein (NifDK), the site of N₂ reduction; alternative nitrogenases using or iron alone exist in some organisms but are less efficient. This pathway accounts for approximately 100-200 million metric tons of fixed nitrogen annually, sustaining global ecosystems by providing ammonia for and synthesis. Ammonia is also generated endogenously through the of nitrogen-containing compounds, particularly via oxidative of in mitochondria. In this process, enzymes such as catalyze the removal of the α-amino group from glutamate, yielding α-ketoglutarate, NADH, and NH₄⁺ (which equilibrates to NH₃ at physiological pH), with the reaction being reversible but favoring under high glutamate concentrations. precedes in many cases, where amino groups from various are transferred to α-ketoglutarate to form glutamate via aminotransferases (e.g., : + α-ketoglutarate → pyruvate + glutamate), followed by glutamate . This catabolic route produces excess ammonia during protein breakdown, especially in or high-protein diets, but rapid accumulation is toxic, necessitating pathways like the in mammals. Additional minor pathways include the hydrolysis of and by glutaminase and , respectively, releasing ammonia: glutamine + H₂O → glutamate + NH₃. These reactions occur in various tissues, such as the and , to regulate pH or provide for local . In anaerobic environments, some produce ammonia via dissimilatory reduction, reducing to ammonia as an electron sink, though this is less common than fixation or globally. Emerging research explores engineered microbial systems for enhanced biological ammonia production from waste or bioresources, but these remain experimental and do not represent dominant natural pathways.

Physiological Functions

In mammals, ammonia serves primarily as an intermediate in nitrogen homeostasis, generated through the deamination of during and , with daily production estimated at 300–500 mmol in humans depending on dietary protein intake. This nitrogenous waste is highly toxic, particularly to the , necessitating rapid detoxification via the hepatic , where ammonia is incorporated into for renal , maintaining systemic nitrogen balance and preventing . Disruptions in this process, as seen in urea cycle disorders, lead to ammonia accumulation exceeding 100 μmol/L, causing through mechanisms including astrocyte swelling and altered . A critical physiological role occurs in the kidneys, where ammonia production from glutamine deamidation in proximal tubule cells facilitates acid-base regulation by buffering secreted hydrogen ions to form ammonium (NH₄⁺), which is excreted in urine. This ammoniagenesis accounts for approximately 30–50% of net renal acid excretion under basal conditions and up to 80% during chronic metabolic acidosis, with production rates increasing 5–10-fold in response to acid loads via upregulated glutaminase and glutamine synthetase activity. In this capacity, ammonia functions not as a waste but as an adaptive buffer, enabling the kidney to excrete excess protons without depleting bicarbonate stores, thus preserving blood pH between 7.35 and 7.45. In the , ammonia participates in the glutamate- cycle, where uptake synaptic glutamate and ammonia to synthesize via , which is then transferred to neurons for reconversion to glutamate, supporting excitatory and preventing . This cycle detoxifies low-level ammonia entering the (typically <50 μmol/L under normoammonemic conditions) while recycling the primary excitatory , with activity tightly regulated to avoid accumulation that could impair neuronal function. Elevated ammonia disrupts this balance by depleting glutamate and α-ketoglutarate, shifting toward synthesis at the expense of production, though physiological ammonia fluxes remain below thresholds for overt . Emerging evidence suggests ammonia may also modulate inhibitory GABA synthesis indirectly through glutamatergic pathways, but such roles require further validation beyond pathological contexts like .

Medical and Therapeutic Applications

Aromatic ammonia spirits, inhaled as , are employed to counteract fainting or syncope by irritating respiratory mucous membranes, thereby stimulating inhalation reflexes and restoring consciousness. This application leverages ammonia's pungent odor and irritant properties to trigger a rapid physiological response, increasing and . Such inhalants have been documented in medical use since at least the and are available over-the-counter, though their in athletics for arousal lacks robust evidence of ergogenic benefits and carries risks of respiratory irritation. Ammonium chloride, a salt derived from ammonia, functions as an expectorant in cough syrups by inducing bronchial irritation that enhances mucus clearance from the airways. It is also administered intravenously as an acidifying agent to treat and associated , where it replenishes chloride and lowers blood pH through conversion to and in the liver. Typical dosing for alkalosis correction involves 0.5–1 mEq/kg over several hours, monitored to avoid . In oncology, ammonia serves as a stabilizing ligand in cisplatin, a platinum(II) complex (cis-[Pt(NH₃)₂Cl₂]) approved for treating testicular, ovarian, bladder, lung, and head/neck cancers since 1978. The coordinated ammonia groups enable selective aquation in low-chloride cellular environments, allowing the platinum to form DNA cross-links that trigger apoptosis in rapidly dividing tumor cells. Analogs like carboplatin retain similar ammine ligands, underscoring ammonia's role in efficacious coordination chemotherapy. Additionally, isotopically labeled ammonia (¹³N-ammonia) is injected for positron emission tomography imaging to assess myocardial perfusion, providing diagnostic insights into cardiac ischemia with high sensitivity. Ammonia also acts as a synthetic precursor for pharmaceuticals such as sulfa drugs and certain vitamins, though direct therapeutic administration is limited by its toxicity.

Extraterrestrial Presence

Interstellar and Planetary Detection

Ammonia was first detected in the in 1968 toward the Sagittarius B2 through its emission lines, marking the initial identification of a polyatomic molecule in space. Observations utilized the 23.7 GHz inversion transition of NH₃, enabling mapping of dense s where ammonia serves as a tracer for kinetic temperatures due to its collisional excitation properties. Subsequent surveys have revealed ammonia abundances of 10⁻⁸ to 10⁻⁷ relative to H₂ in star-forming regions, with detections spanning from nearby clouds like Orion to distant galactic centers. Deuterated isotopologues, such as ND₃ and NHD₂, have been identified more recently in cold, dense cores, providing insights into processes driven by ion-molecule reactions at low temperatures below 20 K. For instance, triply deuterated ammonia (ND₃) was announced in 2002 in a 1,000 light-years away, highlighting rare isotopic enrichments up to 10⁴ times solar values due to successive deuteration pathways. These detections rely on submillimeter from facilities like the Atacama Large Millimeter/submillimeter Array (ALMA), confirming ammonia's role in pre-stellar core chemistry. In the solar system, ammonia has been spectroscopically confirmed in the atmospheres of gas giants, primarily through infrared and visible absorption features. On Jupiter, NH₃ absorption at 647 nm in the visible spectrum and deeper infrared bands indicate upper tropospheric clouds of ammonia ice at pressures around 0.5–1 bar, with Juno spacecraft data from 2020 revealing subsurface enrichment via shallow lightning and "mushball" convection suppressing deep mixing. Saturn exhibits similar NH₃ signatures, though depleted relative to solar abundances due to possible sequestration in deeper layers or photochemical loss. Ice giants and show ammonia-derived haze layers inferred from ultraviolet spectroscopy, with absorption lines confirming trace NH₃ vapor amid methane-dominated atmospheres, though quantities are low due to cold stratospheric photodissociation. On , data from 2019 detected ammonia hydrates on the surface in , likely primordial residues from early icy crust formation, stable against UV and degradation over billions of years. Tentative reports of ammonia in Venus's clouds emerged in 2024 from ground-based observations, but remain unconfirmed amid debates over spectral fitting and potential instrumental artifacts. For exoplanets and planetary-mass objects, ammonia detection lagged until (JWST) observations in 2023–2025, with the first unambiguous NH₃ identification in a late companion using Mid-Infrared Instrument (MIRI) coronagraphy at 10.5 μm absorption. This 2025 detection in a cold atmosphere ( ~800 K) constrains formation mechanisms, as NH₃ persistence indicates low-temperature gas-phase synthesis rather than high-temperature dissociation. Ammonia is modeled as a potential for habitable exoplanets with reducing atmospheres, detectable via transmission spectroscopy if abundances exceed 10 ppm, though abiotic sources like complicate interpretations.

Astrophysical Formation and Significance

Ammonia (NH₃) forms in the (ISM) predominantly via gas-phase ion-molecule reactions under cold conditions (10–100 K), where atomic nitrogen reacts with H₃⁺ to initiate the chain: H₃⁺ + N → NH⁺ + H₂, followed by steps such as NH⁺ + H₂ → NH₂⁺ + H and NH₂⁺ + H₂ → NH₃ + H. These reactions proceed efficiently in dense molecular clouds due to sufficient collision rates and UV shielding from dissociation, with laboratory measurements confirming rate constants around 4.5 × 10⁻¹⁰ cm³ s⁻¹ for key steps at interstellar temperatures. Surface on dust grains contributes marginally, as gas-phase routes dominate observed abundances. Observations of ammonia's ground-state rotational transitions, particularly ortho-NH₃ (J_K = 0_0 → 1_0), reveal its presence in cold cores, protostellar disks, and distant starburst galaxies, with column densities often exceeding 10¹⁴ cm⁻² in dense regions comparable to high-mass star-forming sources. In gravitationally lensed systems at z ≈ 2.6, ammonia emission traces luminosities around 2.8 × 10⁶ L_⊙, representing a fractional contribution of ~2.5 × 10⁻⁷, indicating robust formation even in early environments. Astrophysically, ammonia acts as a thermometer for kinetic temperatures in dense ISM gas (T_K ~ 10–50 K), leveraging its inversion line excitation via H₂ collisions to map thermal structures in molecular clouds and filaments. In massive star formation, dense hot ammonia rings (radii 200–700 AU) around protostars like HW2 signal accretion and outflow dynamics, resolving mechanisms for overcoming radiation pressure barriers. Its deuterium variants, such as ND₃, probe fractionation and nitrogen chemistry, while maser emissions (e.g., NH₃ 9,6) highlight compact, unresolved regions in high-mass forming clusters, aiding models of core collapse and envelope evolution. Ammonia abundances also inform spectroscopic line lists for brown dwarf and cool stellar atmospheres, though ISM diagnostics remain its primary role.

References

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