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Melting point
Melting point
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Ice cubes put in water will start to melt when they reach their melting point of 0 °C

The melting point (or, rarely, liquefaction point) of a substance is the temperature at which it changes state from solid to liquid. At the melting point the solid and liquid phase exist in equilibrium. The melting point of a substance depends on pressure and is usually specified at a standard pressure such as 1 atmosphere or 100 kPa.

When considered as the temperature of the reverse change from liquid to solid, it is referred to as the freezing point or crystallization point. Because of the ability of substances to supercool, the freezing point can easily appear to be below its actual value. When the "characteristic freezing point" of a substance is determined, in fact, the actual methodology is almost always "the principle of observing the disappearance rather than the formation of ice, that is, the melting point."[1]

Examples

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Melting points (in blue) and boiling points (in pink) of the first eight carboxylic acids (°C)

For most substances, melting and freezing points are approximately equal. For example, the melting and freezing points of mercury is 234.32 kelvins (−38.83 °C; −37.89 °F).[2] However, certain substances possess differing solid-liquid transition temperatures. For example, agar melts at 85 °C (185 °F; 358 K) and solidifies from 31 °C (88 °F; 304 K); such direction dependence is known as hysteresis. The melting point of ice at 1 atmosphere of pressure is very close[3] to 0 °C (32 °F; 273 K); this is also known as the ice point. In the presence of nucleating substances, the freezing point of water is not always the same as the melting point. In the absence of nucleators water can exist as a supercooled liquid down to −48.3 °C (−54.9 °F; 224.8 K) before freezing.[4]

The metal with the highest melting point is tungsten, at 3,414 °C (6,177 °F; 3,687 K);[5] this property makes tungsten excellent for use as electrical filaments in incandescent lamps. The often-cited carbon does not melt at ambient pressure but sublimes at about 3,700 °C (6,700 °F; 4,000 K); a liquid phase only exists above pressures of 10 MPa (99 atm) and estimated 4,030–4,430 °C (7,290–8,010 °F; 4,300–4,700 K) (see carbon phase diagram). Hafnium carbonitride (HfCN) is a refractory compound with the highest known melting point of any substance to date and the only one confirmed to have a melting point above 4,273 K (4,000 °C; 7,232 °F) at ambient pressure. Quantum mechanical computer simulations predicted that this alloy (HfN0.38C0.51) would have a melting point of about 4,400 K.[6] This prediction was later confirmed by experiment, though a precise measurement of its exact melting point has yet to be confirmed.[7] At the other end of the scale, helium does not freeze at all at normal pressure even at temperatures arbitrarily close to absolute zero; a pressure of more than twenty times normal atmospheric pressure is necessary.

List of common chemicals
Chemical[I] Density (g/cm3) Melt (K)[8] Boil (K)
Water @STP 1 273 373
Solder (Pb60Sn40) 461
Cocoa butter 307.2 -
Paraffin wax 0.9 310 643
Hydrogen 0.00008988 14.01 20.28
Helium 0.0001785 [II] 4.22
Beryllium 1.85 1,560 2,742
Carbon 2.267 [III][9] 4,000[III][9]
Nitrogen 0.0012506 63.15 77.36
Oxygen 0.001429 54.36 90.20
Sodium 0.971 370.87 1,156
Magnesium 1.738 923 1,363
Aluminium 2.698 933.47 2,792
Sulfur 2.067 388.36 717.87
Chlorine 0.003214 171.6 239.11
Potassium 0.862 336.53 1,032
Titanium 4.54 1,941 3,560
Iron 7.874 1,811 3,134
Nickel 8.912 1,728 3,186
Copper 8.96 1,357.77 2,835
Zinc 7.134 692.88 1,180
Gallium 5.907 302.9146 2,673
Silver 10.501 1,234.93 2,435
Cadmium 8.69 594.22 1,040
Indium 7.31 429.75 2,345
Iodine 4.93 386.85 457.4
Tantalum 16.654 3,290 5,731
Tungsten 19.25 3,695 5,828
Platinum 21.46 2,041.4 4,098
Gold 19.282 1,337.33 3,129
Mercury 13.5336 234.43 629.88
Lead 11.342 600.61 2,022
Bismuth 9.807 544.7 1,837

Notes

  1. ^ Z is the standard symbol for atomic number; C is the standard symbol for heat capacity; and χ is the standard symbol for electronegativity on the Pauling scale.
  2. ^ Helium does not solidify at a pressure of one atmosphere. Helium can only solidify at pressures above 25 atmospheres, which corresponds to a melting point of absolute zero.
  3. ^ a b Carbon does not melt at any temperature under standard pressure, instead it sublimes around 4,100 K

Melting point measurements

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Kofler bench with samples for calibration

Many laboratory techniques exist for the determination of melting points. A Kofler bench is a metal strip with a temperature gradient (range from room temperature to 300 °C). Any substance can be placed on a section of the strip, revealing its thermal behaviour at the temperature at that point. Differential scanning calorimetry gives information on melting point together with its enthalpy of fusion.

Automatic digital melting point meter

A basic melting point apparatus for the analysis of crystalline solids consists of an oil bath with a transparent window (most basic design: a Thiele tube) and a simple magnifier. Several grains of a solid are placed in a thin glass tube and partially immersed in the oil bath. The oil bath is heated (and stirred) and with the aid of the magnifier (and external light source) melting of the individual crystals at a certain temperature can be observed. A metal block might be used instead of an oil bath. Some modern instruments have automatic optical detection.

The measurement can also be made continuously with an operating process. For instance, oil refineries measure the freeze point of diesel fuel "online", meaning that the sample is taken from the process and measured automatically. This allows for more frequent measurements as the sample does not have to be manually collected and taken to a remote laboratory.[citation needed]

Techniques for refractory materials

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For refractory materials (e.g. platinum, tungsten, tantalum, some carbides and nitrides, etc.) the extremely high melting point (typically considered to be above, say, 1,800 °C) may be determined by heating the material in a black body furnace and measuring the black-body temperature with an optical pyrometer. For the highest melting materials, this may require extrapolation by several hundred degrees. The spectral radiance from an incandescent body is known to be a function of its temperature. An optical pyrometer matches the radiance of a body under study to the radiance of a source that has been previously calibrated as a function of temperature. In this way, the measurement of the absolute magnitude of the intensity of radiation is unnecessary. However, known temperatures must be used to determine the calibration of the pyrometer. For temperatures above the calibration range of the source, an extrapolation technique must be employed. This extrapolation is accomplished by using Planck's law of radiation. The constants in this equation are not known with sufficient accuracy, causing errors in the extrapolation to become larger at higher temperatures. However, standard techniques have been developed to perform this extrapolation.[citation needed]

Consider the case of using gold as the source (mp = 1,063 °C). In this technique, the current through the filament of the pyrometer is adjusted until the light intensity of the filament matches that of a black-body at the melting point of gold. This establishes the primary calibration temperature and can be expressed in terms of current through the pyrometer lamp. With the same current setting, the pyrometer is sighted on another black-body at a higher temperature. An absorbing medium of known transmission is inserted between the pyrometer and this black-body. The temperature of the black-body is then adjusted until a match exists between its intensity and that of the pyrometer filament. The true higher temperature of the black-body is then determined from Planck's Law. The absorbing medium is then removed and the current through the filament is adjusted to match the filament intensity to that of the black-body. This establishes a second calibration point for the pyrometer. This step is repeated to carry the calibration to higher temperatures. Now, temperatures and their corresponding pyrometer filament currents are known and a curve of temperature versus current can be drawn. This curve can then be extrapolated to very high temperatures.

In determining melting points of a refractory substance by this method, it is necessary to either have black body conditions or to know the emissivity of the material being measured. The containment of the high melting material in the liquid state may introduce experimental difficulties. Melting temperatures of some refractory metals have thus been measured by observing the radiation from a black body cavity in solid metal specimens that were much longer than they were wide. To form such a cavity, a hole is drilled perpendicular to the long axis at the center of a rod of the material. These rods are then heated by passing a very large current through them, and the radiation emitted from the hole is observed with an optical pyrometer. The point of melting is indicated by the darkening of the hole when the liquid phase appears, destroying the black body conditions. Today, containerless laser heating techniques, combined with fast pyrometers and spectro-pyrometers, are employed to allow for precise control of the time for which the sample is kept at extreme temperatures. Such experiments of sub-second duration address several of the challenges associated with more traditional melting point measurements made at very high temperatures, such as sample vaporization and reaction with the container.

Thermodynamics

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Pressure dependence of water melting point.

For a solid to melt, heat is required to raise its temperature to the melting point. However, further heat needs to be supplied for the melting to take place: this is called the heat of fusion, and is an example of latent heat.[10]

From a thermodynamics point of view, at the melting point the change in Gibbs free energy (ΔG) of the material is zero, but the enthalpy (H) and the entropy (S) of the material are increasing (ΔH, ΔS > 0). Melting phenomenon happens when the Gibbs free energy of the liquid becomes lower than the solid for that material. At various pressures this happens at a specific temperature. It can also be shown that:

Here T, ΔS and ΔH are respectively the temperature at the melting point, change of entropy of melting and the change of enthalpy of melting.

The melting point is sensitive to extremely large changes in pressure, but generally this sensitivity is orders of magnitude less than that for the boiling point, because the solid-liquid transition represents only a small change in volume.[11][12] If, as observed in most cases, a substance is more dense in the solid than in the liquid state, the melting point will increase with increases in pressure. Otherwise the reverse behavior occurs. Notably, this is the case of water, as illustrated graphically to the right, but also of Si, Ge, Ga, Bi. With extremely large changes in pressure, substantial changes to the melting point are observed. For example, the melting point of silicon at ambient pressure (0.1 MPa) is 1415 °C, but at pressures in excess of 10 GPa it decreases to 1000 °C.[13]

Melting points are often used to characterize organic and inorganic compounds and to ascertain their purity. The melting point of a pure substance is always higher and has a smaller range than the melting point of an impure substance or, more generally, of mixtures. The higher the quantity of other components, the lower the melting point and the broader will be the melting point range, often referred to as the "pasty range". The temperature at which melting begins for a mixture is known as the solidus while the temperature where melting is complete is called the liquidus. Eutectics are special types of mixtures that behave like single phases. They melt sharply at a constant temperature to form a liquid of the same composition. Alternatively, on cooling a liquid with the eutectic composition will solidify as uniformly dispersed, small (fine-grained) mixed crystals with the same composition.

In contrast to crystalline solids, glasses do not possess a melting point; on heating they undergo a smooth glass transition into a viscous liquid. Upon further heating, they gradually soften, which can be characterized by certain softening points.

Freezing-point depression

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The freezing point of a solvent is depressed when another compound is added, meaning that a solution has a lower freezing point than a pure solvent. This phenomenon is used in technical applications to avoid freezing, for instance by adding salt or ethylene glycol to water.[citation needed]

Carnelley's rule

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In organic chemistry, Carnelley's rule, established in 1882 by Thomas Carnelley, states that high molecular symmetry is associated with high melting point.[14] Carnelley based his rule on examination of 15,000 chemical compounds. For example, for three structural isomers with molecular formula C5H12 the melting point increases in the series isopentane −160 °C (113 K) n-pentane −129.8 °C (143 K) and neopentane −16.4 °C (256.8 K).[15] Likewise in xylenes and also dichlorobenzenes the melting point increases in the order meta, ortho and then para. Pyridine has a lower symmetry than benzene hence its lower melting point but the melting point again increases with diazine and triazines. Many cage-like compounds like adamantane and cubane with high symmetry have relatively high melting points.

A high melting point results from a high heat of fusion, a low entropy of fusion, or a combination of both. In highly symmetrical molecules the crystal phase is densely packed with many efficient intermolecular interactions resulting in a higher enthalpy change on melting.

Like many high symmetry compounds, tetrakis(trimethylsilyl)silane has a very high melting point (m.p.) of 319-321 °C. It tends to sublime, so the m.p. determination requires that the sample be sealed in a tube.[16]

Predicting the melting point of substances (Lindemann's criterion)

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An attempt to predict the bulk melting point of crystalline materials was first made in 1910 by Frederick Lindemann.[17] The idea behind the theory was the observation that the average amplitude of thermal vibrations increases with increasing temperature. Melting initiates when the amplitude of vibration becomes large enough for adjacent atoms to partly occupy the same space. The Lindemann criterion states that melting is expected when the vibration root mean square amplitude exceeds a threshold value.

Assuming that all atoms in a crystal vibrate with the same frequency ν, the average thermal energy can be estimated using the equipartition theorem as[18]

where m is the atomic mass, ν is the frequency, u is the average vibration amplitude, kB is the Boltzmann constant, and T is the absolute temperature. If the threshold value of u2 is c2a2 where c is the Lindemann constant and a is the atomic spacing, then the melting point is estimated as

Several other expressions for the estimated melting temperature can be obtained depending on the estimate of the average thermal energy. Another commonly used expression for the Lindemann criterion is[19]

From the expression for the Debye frequency for ν,

where θD is the Debye temperature and h is the Planck constant. Values of c range from 0.15 to 0.3 for most materials.[20]

Databases and automated prediction

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In February 2011, Alfa Aesar released over 10,000 melting points of compounds from their catalog as open data[21] and similar data has been mined from patents.[22] The Alfa Aesar and patent data have been summarized in (respectively) random forest[21] and support vector machines.[22]

Melting point of the elements

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See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
The melting point of a substance is the specific at which it transitions from a to a state under standard , where the solid and liquid phases coexist in . For pure, crystalline substances, this occurs at a precise, characteristic that serves as a fundamental for identification and purity assessment. In contrast, impure or non-crystalline materials exhibit a melting range rather than a sharp point, with the transition beginning and ending over a broader interval. This property is influenced by several factors, including the presence of impurities, which lower the melting point and widen the range due to colligative effects disrupting the crystal lattice; molecular structure, where stronger intermolecular forces like hydrogen bonding or ionic interactions raise the melting point; and external pressure, which generally increases the melting point for most substances following the Clapeyron equation, though the effect is minimal at standard conditions. Melting points play a critical role across scientific and industrial domains: in for verifying compound identity and purity during synthesis; in for designing alloys, polymers, and ceramics with desired thermal behaviors; and in pharmaceuticals for ensuring drug stability and formulation efficacy, where precise measurement techniques like tube methods or are employed.

Fundamentals

Definition and Phase Transition

The melting point of a substance is defined as the at which the solid and phases coexist in , typically measured at standard atmospheric pressure of 1 atm, marking the point where the solid begins to transform into a without further increase until the phase change is complete. This characteristic is a fundamental for pure, crystalline solids, reflecting the conditions under which the of the two phases is equal (ΔG = 0 at T_m), allowing both phases to exist stably. Melting represents a first-order , characterized by a discontinuous change in properties such as volume and , accompanied by the absorption of known as the (ΔH_fus). During this process, the solid's ordered molecular structure breaks down into the more disordered liquid state, resulting in an increase in (ΔS_fus > 0), where the entropy change is related to the by ΔS_fus = ΔH_fus / T_m at the equilibrium . The transition occurs at constant and , with the system requiring energy input to overcome intermolecular forces, leading to the absorption without a rise in . The slope of the melting curve in the phase diagram, which describes how the melting point varies with pressure, is given by the Clapeyron equation: dTdP=ΔVΔS\frac{dT}{dP} = \frac{\Delta V}{\Delta S} where ΔV is the change in molar volume from solid to liquid (typically positive for most substances) and ΔS is the entropy change during fusion. This relation highlights the interdependence of temperature and pressure at equilibrium, with increasing pressure generally raising the melting point for materials where the liquid occupies more volume than the solid. Early observations of melting points contributed to the development of temperature scales; in 1714, calibrated his mercury using the melting point of at 32°F as a fixed reference, alongside other reproducible thermal events, establishing a basis for precise thermometry.

Importance in Science and Industry

In science, the melting point serves as a key indicator of the strength of intermolecular forces within a substance, with higher melting points generally reflecting stronger attractive forces that require more energy to overcome for . It plays a central role in constructing phase diagrams, where the melting curve delineates the boundary between and liquid phases under varying temperature and pressure conditions, aiding in the prediction of material behavior. Additionally, melting points are integral to cryoscopy, the study of in solutions, which leverages the relationship between solute concentration and lowered melting temperatures to determine molecular weights and solute properties. These applications collectively enhance the understanding of molecular structures, as deviations in melting points from expected values reveal insights into purity, polymorphism, or structural irregularities in compounds. In industry, melting points are essential for metallurgy, where they guide alloy design by influencing casting processes, phase stability, and the selection of compositions that achieve desired mechanical properties without unintended melting during use. In pharmaceuticals, the melting point assesses drug stability and purity, ensuring that active ingredients withstand processing temperatures without degradation, particularly for high-melting-point compounds prone to instability during melt extrusion. It also indicates the thermal resilience of drug lattices, informing formulation strategies to maintain efficacy over time. Food science relies on melting points to optimize processing temperatures for fats, oils, and confectionery, enabling quality control in products like chocolate—where precise melting ensures texture and shelf stability—and dairy items, preventing adulteration or inconsistent melting behavior. In electronics, high melting points of materials like silicon (1414°C) are critical for semiconductor fabrication, allowing wafers to endure high-temperature doping and annealing without structural failure. Environmentally, melting points underpin climate science by defining thresholds for ice sheet stability; for instance, the gradual melting of and ice sheets, driven by rising temperatures exceeding their equilibrium points, has contributed approximately one-third to global sea-level rise observed from 2006 to 2015. This process amplifies risks and disruptions as influx alters ocean dynamics. The economic implications of melting points are profound in for demanding sectors like , where high-melting-point alloys enable engine components to operate under extreme heat, reducing maintenance costs and enhancing —potentially lowering overall production expenses by optimizing , durable designs. Such choices drive innovations in high-temperature environments, balancing performance gains against energy-intensive manufacturing to achieve long-term cost savings.

Examples and Data

Common Substances

The melting point serves as a fundamental benchmark for phase transitions in common materials, illustrating how drives the shift from solid to states under standard . For organic compounds, exemplifies this with its precise melting point of 0°C, where transitions to , a value critical for environmental and biological processes. , the primary component of table sugar, melts at 186°C, though it often decomposes slightly before fully liquefying, highlighting the thermal sensitivity of carbohydrates. , used in candles and coatings, typically melts around 60°C, providing a low-temperature example of hydrocarbon-based solids that soften gradually over a range due to molecular weight variations. Metals demonstrate higher melting points tied to their strength, influencing applications from to . Iron melts at 1538°C, a temperature that defines production thresholds and industrial forging limits. Aluminum, valued for its lightweight properties, reaches its melting point at 660°C, enabling efficient and in . Gold, prized for jewelry, melts at 1064°C, reflecting its resistance to oxidation and stability at elevated temperatures. Polymers like polyethylene illustrate the diversity in synthetic materials, with a melting point around 115°C for low-density variants, which broadens the utility of plastics in packaging while limiting their use in high-heat environments. This range underscores how chain branching affects thermal behavior in polymers.
SubstanceMelting Point (°C)Notes
Water (ice)0Benchmark for aqueous phase equilibrium.
Sucrose186Decomposes near melting.
Paraffin wax~60Varies by composition (47–65°C range).
Iron1538Key for metallurgy.
Aluminum660Enables low-energy processing.
Gold1064High purity standard.
Polyethylene (LDPE)~115Represents plastic softening range.
Melting points can vary significantly based on purity and structural forms; impurities lower the temperature and widen the melting range by disrupting crystal lattice integrity, as seen in contaminated samples melting several degrees below pure counterparts. Polymorphic forms of the same element, such as carbon's (melting near 3550°C under ) versus (which sublimes at ~3650°C without melting at ), further demonstrate how atomic arrangements dictate thermal stability.

Melting Points of Elements

The melting points of the chemical elements span an enormous range, reflecting the diversity of bonding types and atomic structures across the periodic table. exhibits the lowest melting point at 0.95 K (under ~25 atm pressure), while has the highest at 3695 K (3422 °C). These extremes highlight how elements transition from gases and liquids at standard conditions to solids capable of withstanding extreme temperatures. Periodic trends in melting points are pronounced, particularly among metals. For transition metals, melting points generally increase across a period due to stronger as decreases and the number of delocalized electrons rises, enhancing lattice stability. Notable anomalies include mercury, with a melting point of -38.8 °C (234.3 K), resulting from relativistic effects that contract the 6s orbital and weaken . Nonmetals and metalloids often show lower values due to covalent or molecular structures, such as carbon's sublimate behavior, but graphite's effective melting point exceeds 4000 K under pressure. Several factors influence these melting points. Smaller atomic radii in later periods strengthen interatomic forces, while higher in nonmetals favors directional covalent bonds over isotropic metallic ones, typically lowering melting points. plays a key role; for instance, body-centered cubic (BCC) lattices in metals like provide higher coordination and thus elevated melting points compared to face-centered cubic (FCC) structures in elements like . The following table lists the melting points of all 118 known elements, ordered by , with values in both and . Data are drawn from standard compilations and represent normal melting points at standard unless otherwise noted (e.g., requires pressure >1 ; elements like carbon and sublime at 1 ). Values for elements (atomic numbers 104–118) are largely theoretical or estimated due to their short half-lives and synthetic nature; melting points have not been experimentally determined as of 2025.
Atomic NumberSymbolElementMelting Point (°C)Melting Point (K)
1HHydrogen-259.1614.01
2HeHelium-272.20 (0.95 at ~25 atm)0.95 (at ~25 atm)
3LiLithium180.54453.69
4BeBeryllium12871560
5BBoron20762349
6CCarbonSublimes ~3650 (graphite at 1 atm; diamond ~3550 under high P)~3923 (graphite); ~3823 (diamond under P)
7NNitrogen-210.0063.15
8OOxygen-218.7954.36
9FFluorine-219.6753.48
10NeNeon-248.5924.56
11NaSodium97.72370.87
12MgMagnesium650.00923.15
13AlAluminum660.32933.47
14SiSilicon14141687
15PPhosphorus44.15 (white)317.30
16SSulfur115.21 (rhombic)388.36
17ClChlorine-100.98172.17
18ArArgon-189.3483.81
19KPotassium63.28336.43
20CaCalcium8421115
21ScScandium15411814
22TiTitanium16681941
23VVanadium19102183
24CrChromium19072180
25MnManganese12461519
26FeIron15381811
27CoCobalt14951768
28NiNickel14551728
29CuCopper1084.621357.77
30ZnZinc419.53692.68
31GaGallium29.76302.91
32GeGermanium938.251211.40
33AsArsenicSublimes 615 (gray at 1 atm; 817 at 36 atm)888 (subl.); 1090 (at 36 atm)
34SeSelenium221494
35BrBromine-7.2265.95
36KrKrypton-157.4115.75
37RbRubidium39.31312.46
38SrStrontium7771050
39YYttrium15221795
40ZrZirconium18552128
41NbNiobium24772750
42MoMolybdenum26232896
43TcTechnetium21572430
44RuRuthenium23342607
45RhRhodium19642237
46PdPalladium15551828
47AgSilver961.781234.93
48CdCadmium320.99594.14
49InIndium156.60429.75
50SnTin231.93 (white)505.08
51SbAntimony630.63903.78
52TeTellurium449.51722.66
53IIodine113.70386.85
54XeXenon-111.75161.40
55CsCesium28.44301.59
56BaBarium7271000
57LaLanthanum9201193
58CeCerium7951068
59PrPraseodymium9311204
60NdNeodymium10211294
61PmPromethium10421315
62SmSamarium10721345
63EuEuropium8221095
64GdGadolinium13131586
65TbTerbium13561629
66DyDysprosium14121685
67HoHolmium14741747
68ErErbium15291802
69TmThulium15451818
70YbYtterbium8241097
71LuLutetium16631936
72HfHafnium22332506
73TaTantalum30173290
74WTungsten34223695
75ReRhenium31863459
76OsOsmium30333306
77IrIridium24462719
78PtPlatinum1768.32041.45
79AuGold1064.181337.33
80HgMercury-38.83234.32
81TlThallium304577
82PbLead327.46600.61
83BiBismuth271.40544.55
84PoPolonium254527
85AtAstatine302 (est.)575 (est.)
86RnRadon-71 (est.)202 (est.)
87FrFrancium27 (est.)300 (est.)
88RaRadium700 (est.)973 (est.)
89AcActinium10501323
90ThThorium17502023
91PaProtactinium15721845
92UUranium11321405
93NpNeptunium644917
94PuPlutonium640913
95AmAmericium9941267
96CmCurium13401613
97BkBerkelium9861259
98CfCalifornium900 (est.)1173 (est.)
99EsEinsteinium860 (est.)1133 (est.)
100FmFermium1527 (est.)1800 (est.)
101MdMendelevium
102NoNobelium827 (est.)1100 (est.)
103LrLawrencium
104RfRutherfordium
105DbDubnium
106SgSeaborgium
107BhBohrium
108HsHassium
109MtMeitnerium
110DsDarmstadtium
111RgRoentgenium
112CnCopernicium
113NhNihonium
114FlFlerovium
115McMoscovium
116LvLivermorium
117TsTennessine
118OgOganesson
Note: Allotropes affect melting points (e.g., white phosphorus at 44.15°C vs. >600°C; white tin at 232°C vs. gray ~13°C); values here use standard forms where applicable.

Record Holders

The lowest known melting point among substances is that of helium at 0.95 K under approximately 25 atm pressure. Among pure elements, helium holds the record for the lowest melting point, while tungsten has the highest melting point of any element that melts under standard conditions at 3422 °C (3695 K); carbon sublimes at around 3915 °C without melting. The highest known melting point is held by tantalum hafnium carbide alloy (such as Ta4_4HfC5_5), reported at 3990 °C (4263 K).

Measurement Methods

Experimental Techniques

The tube technique is a classical method widely used for determining the melting points of organic compounds, particularly those with low to moderate melting temperatures. In this approach, a small sample of the finely powdered solid is packed into a thin tube, typically 1-2 mm in height, and the sealed end of the tube is inserted into a controlled heating block or . The temperature is raised gradually at a rate of 1-2°C per minute to ensure equilibrium, and the melting point is observed visually through a magnifying lens or as the point when the sample first liquefies and forms a meniscus at the bottom of the tube, with the final melting point noted when the entire sample has melted. This method provides a melting range rather than a single point, allowing for assessment of sample behavior during the from solid to liquid. Hot stage microscopy offers a complementary visual technique for melting point determination, especially useful for observing morphological changes in samples. The method involves placing a small amount of sample on a mounted on a heated stage, where the temperature is programmed to increase linearly while the sample is viewed under a polarizing . is identified by the disappearance of or the formation of a phase, providing detailed insights into alterations during the transition. This technique is particularly effective for small samples or those requiring to detect subtle phase changes. Calorimetric methods, such as differential scanning calorimetry (DSC), provide a quantitative approach by measuring the heat flow associated with the endothermic melting process. In DSC, the sample and a reference material are heated at a constant rate in separate crucibles, and the difference in heat flow is recorded as a function of temperature; the melting point TmT_m is determined from the extrapolated onset temperature of the endothermic peak, where the baseline intersects the tangent to the peak's leading edge. This yields precise thermodynamic data, including the enthalpy of fusion from the peak area. DSC is favored for its sensitivity and ability to handle milligram-scale samples./04:Differential_Scanning_Calorimetry(DSC)) Purity assessment is integral to these techniques, as a sharp melting range (typically less than 0.5-1°C) indicates high purity, while impurities cause a depression and broadening of the range due to colligative effects that lower the at which the last solid dissolves in the melt. For instance, in the capillary method, pure samples melt over a narrow interval, whereas impure ones exhibit a gradual softening over several degrees. Similar observations apply in DSC, where peak sharpness correlates with purity levels above 99%./05:_HOW_TO_INTERPRET_YOUR_RESULTS/5.03:_MELTING_POINT_ANALYSIS-_IDENTITY_AND_PURITY) Precision in melting point measurements relies on standardized protocols, such as those outlined in ASTM E324 for the capillary tube method, which ensure through controlled heating rates and calibrated , achieving inter-laboratory agreement within 0.5-1°C for pure organics. Common error sources include excessively rapid heating, which causes thermal lag between the sample and thermometer (leading to readings 2-5°C higher than actual), poor sample packing resulting in uneven heating, and effects in some systems where the melt does not fully transition without aids. To mitigate these, slow ramp rates and triplicate measurements are recommended.

Challenges for High-Temperature Materials

Refractory materials, such as tungsten with a melting point of approximately 3420°C and hafnium carbide at around 3950°C, pose significant challenges for melting point determination due to their extreme thermal stability, often exceeding 2000°C, which surpasses the capabilities of conventional furnaces and crucibles that would themselves melt or react chemically. These substances, including carbon in forms like graphite that sublimes near 3600°C under certain conditions, require specialized techniques to avoid contamination and enable accurate observation of phase transitions. Advanced methods have been developed to address these issues, including levitation melting techniques that suspend samples without physical contact to prevent container reactions. Electromagnetic levitation uses alternating magnetic fields to levitate and heat conductive metals like tungsten, allowing undercooling and precise thermophysical measurements up to 3000 K without crucible interference. Acoustic levitation, employing ultrasonic waves, is particularly useful for dielectric refractory oxides and non-conductive materials, enabling containerless processing and density measurements of melts at temperatures exceeding 2000°C. Laser heating within diamond anvil cells (LHDAC) combines high-pressure compression with focused laser beams to achieve and sustain temperatures over 4000 K, facilitating in situ studies of melting in refractory metals like tantalum and hafnium compounds via X-ray diffraction. Optical pyrometry provides non-contact temperature assessment in these setups by analyzing thermal radiation, though it requires calibration to account for emissivity variations at ultra-high temperatures. Historically, solar furnaces emerged as early solutions for high-temperature experimentation, with facilities like the Odeillo furnace in achieving fluxes up to 10 MW/m² to melt refractories like without electrical input, dating back to mid-20th-century developments for materials testing. Modern advancements incorporate synchrotron-based imaging for real-time observation of melting dynamics, using high-speed X-ray radiography to detect volume changes and phase boundaries in samples under extreme conditions, such as at 2 GPa and temperatures above 2000 K. Despite these innovations, limitations persist, including severe reactions between samples and any containing materials, leading to impure melts and inaccurate data, as seen in early crucible-based attempts with . Vaporization effects at ultra-high temperatures complicate equilibrium measurements, while uncertainties in pyrometric readings for materials like arise from non-ideal blackbody behavior and thermal gradients, resulting in reported melting points with errors up to several hundred . These challenges underscore the need for ongoing refinements in containerless and spectroscopic techniques to achieve reliable determinations for such extreme materials.

Thermodynamic Foundations

Thermodynamic Principles

The melting point TmT_m of a pure substance marks the temperature at which the solid and liquid phases coexist in under a given . This equilibrium condition is governed by the change for the fusion process, where ΔGfus=0\Delta G_\text{fus} = 0. The is expressed as ΔGfus=ΔHfusTmΔSfus\Delta G_\text{fus} = \Delta H_\text{fus} - T_m \Delta S_\text{fus}, leading to the relation Tm=ΔHfusΔSfusT_m = \frac{\Delta H_\text{fus}}{\Delta S_\text{fus}}, with ΔHfus\Delta H_\text{fus} as the and ΔSfus\Delta S_\text{fus} as the entropy of fusion. The ΔHfus\Delta H_\text{fus} quantifies the energy input needed to overcome the cohesive forces in the lattice, enabling the transition to a with greater molecular mobility and weakened bonding. This energy primarily accounts for the disruption of ordered arrangements, such as breaking van der Waals interactions in molecular solids or metallic bonds in elements. For approximation, Richardson's rule posits that ΔSfus[R](/page/R)\Delta S_\text{fus} \approx [R](/page/R) (where [R](/page/R)=8.314[R](/page/R) = 8.314 J/mol·K is the ) for many metals, implying a near-constant increase upon due to configurational disorder. This rule stems from observations that the gain is modest compared to vaporization, reflecting limited volume expansion and primarily rotational or translational freedom in the . An analogous concept to Trouton's rule for boiling—where ΔSvap/Tb85\Delta S_\text{vap} / T_b \approx 85 J/mol·K—applies loosely to fusion, with ΔSfus\Delta S_\text{fus} typically ranging from [R](/page/R)[R](/page/R) to 3[R](/page/R)3[R](/page/R), underscoring the smaller disorder increase during . In diagrams for two-component systems, the is depicted as regions of stable phases separated by boundary lines, with the curves defining behaviors. A eutectic point emerges where the mixture of two components melts congruently at a minimum temperature lower than either pure component's TmT_m, illustrating how compositional variations can shift equilibrium conditions. From a quantum mechanical viewpoint, the approach to melting involves the excitation of lattice vibrational modes (phonons) in the solid, where amplifies anharmonic oscillations, destabilizing the as amplitudes exceed a critical threshold. This vibrational contribution dominates the ΔSfus\Delta S_\text{fus}, with quantum effects becoming prominent in low-temperature or light-element solids where zero-point motion influences lattice stability.

Effects of Pressure and Impurities

The effect of pressure on the melting point of a substance is described by the Clapeyron equation, which relates the change in melting temperature TmT_m with pressure PP to the differences in molar volume and enthalpy of fusion: dTmdP=Tm(VliquidVsolid)ΔHfus,\frac{dT_m}{dP} = \frac{T_m (V_\text{liquid} - V_\text{solid})}{\Delta H_\text{fus}}, where VliquidV_\text{liquid} and VsolidV_\text{solid} are the molar volumes of the liquid and solid phases, respectively, and ΔHfus\Delta H_\text{fus} is the enthalpy of fusion. For most substances, the liquid phase has a larger molar volume than the solid (Vliquid>VsolidV_\text{liquid} > V_\text{solid}), resulting in a positive dTm/dPdT_m/dP and an increase in melting point with applied pressure, as the higher pressure favors the denser solid phase. An exception occurs for water, where ice has a lower density than liquid water (Vliquid<VsolidV_\text{liquid} < V_\text{solid}), leading to a negative dTm/dPdT_m/dP and a decrease in melting point under pressure; for instance, the melting point of ice drops by approximately 0.0075°C per atmosphere increase. Impurities lower the melting point of a pure substance through freezing-point depression, a colligative property that depends on the number of solute particles rather than their identity, applicable to dilute ideal solutions. This depression arises from Raoult's law, which states that the vapor pressure of the solvent over the solution is reduced by the mole fraction of the solute (P=xsolventPP = x_\text{solvent} P^\circ), shifting the solid-liquid equilibrium to a lower temperature to restore equality between the vapor pressures of the solid and solution phases./13%3A_Solutions/13.06%3A_Colligative_Properties-_Freezing_Point_Depression_Boiling_Point_Elevation_and_Osmosis) The magnitude of the depression is given by ΔTm=Kfm\Delta T_m = K_f m, where KfK_f is the cryoscopic constant of the solvent and mm is the molality of the solution; for water, Kf=1.86K_f = 1.86^\circC kg/mol./13%3A_Solutions/13.06%3A_Colligative_Properties-_Freezing_Point_Depression_Boiling_Point_Elevation_and_Osmosis) Mechanistically, the presence of solute increases the entropy of the liquid phase relative to the pure solid, making the liquid state more stable at temperatures where the pure substance would freeze, thus requiring a lower temperature to achieve equilibrium. A practical example is the addition of sodium chloride (NaCl) to ice, where the eutectic mixture at 23 wt% NaCl has a melting point of -21°C, significantly below that of pure ice at 0°C. At extreme pressures, such as those exceeding hundreds of gigapascals, the melting behavior of substances like water ice undergoes profound changes, often studied using (DACs) that compress samples between diamond tips while enabling in situ measurements via X-ray diffraction or . These DAC experiments have mapped melting curves for metals like , , and up to 290 GPa and thousands of , revealing steeper increases in melting temperature due to enhanced atomic interactions under compression. In the case of , high-pressure studies in DACs have identified superionic phases, such as ice XVIII, where the oxygen atoms form a body-centered cubic lattice while protons become highly mobile, resembling a fluid within a solid framework; these phases emerge above approximately 50 GPa and 2000 K, potentially influencing the interiors of icy planets like and .

Prediction and Empirical Rules

Lindemann's Criterion

Lindemann's criterion proposes that a crystalline solid melts when the root-mean-square (RMS) displacement of atoms from their equilibrium lattice positions reaches approximately 10-15% of the average interatomic distance. This threshold, often expressed as the Lindemann parameter δ=u2/a0.100.15\delta = \sqrt{\langle u^2 \rangle}/a \approx 0.10 - 0.15
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