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Density
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Density
A test tube holding four non-miscible colored liquids with different densities
Common symbols
ρ, D, d
SI unitkg/m3
Other units
g/cm3
Extensive?No
Intensive?Yes
Conserved?No
Derivations from
other quantities
Dimension

Density (volumetric mass density or specific mass) is the ratio of a substance's mass to its volume. The symbol most often used for density is ρ (the lower case Greek letter rho), although the Latin letter D (or d) can also be used:[1] where ρ is the density, m is the mass, and V is the volume. In some cases (for instance, in the United States oil and gas industry), density is loosely defined as its weight per unit volume,[2] although this is scientifically inaccurate – this quantity is more specifically called specific weight.

For a pure substance, the density is equal to its mass concentration. Different materials usually have different densities, and density may be relevant to buoyancy, purity and packaging. Osmium is the densest known element at standard conditions for temperature and pressure.

To simplify comparisons of density across different systems of units, it is sometimes replaced by the dimensionless quantity "relative density" or "specific gravity", i.e. the ratio of the density of the material to that of a standard material, usually water. Thus a relative density less than one relative to water means that the substance floats in water.

The density of a material varies with temperature and pressure. This variation is typically small for solids and liquids but much greater for gases. Increasing the pressure on an object decreases the volume of the object and thus increases its density. Increasing the temperature of a substance while maintaining a constant pressure decreases its density by increasing its volume (with a few exceptions). In most fluids, heating the bottom of the fluid results in convection due to the decrease in the density of the heated fluid, which causes it to rise relative to denser unheated material.

The reciprocal of the density of a substance is occasionally called its specific volume, a term sometimes used in thermodynamics. Density is an intensive property in that increasing the amount of a substance does not increase its density; rather it increases its mass.

Other conceptually comparable quantities or ratios include specific density, relative density (specific gravity), and specific weight.

The concept of mass density is generalized in the International System of Quantities to volumic quantities, the quotient of any physical quantity and volume,[3], such as charge density or volumic electric charge.[4]

History

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Density, floating, and sinking

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The understanding that different materials have different densities, and of a relationship between density, floating, and sinking must date to prehistoric times. Much later it was put in writing. Aristotle, for example, wrote:[5]

There is so great a difference in density between salt and fresh water that vessels laden with cargoes of the same weight almost sink in rivers, but ride quite easily at sea and are quite seaworthy. And an ignorance of this has sometimes cost people dear who load their ships in rivers. The following is a proof that the density of a fluid is greater when a substance is mixed with it. If you make water very salt by mixing salt in with it, eggs will float on it. ... If there were any truth in the stories they tell about the lake in Palestine it would further bear out what I say. For they say if you bind a man or beast and throw him into it he floats and does not sink beneath the surface.

— Aristotle, Meteorologica, Book II, Chapter III

Volume vs. density; volume of an irregular shape

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In a well-known but probably apocryphal tale, Archimedes was given the task of determining whether King Hiero's goldsmith was embezzling gold during the manufacture of a golden wreath dedicated to the gods and replacing it with another, cheaper alloy.[6] Archimedes knew that the irregularly shaped wreath could be crushed into a cube whose volume could be calculated easily and compared with the mass; but the king did not approve of this. Baffled, Archimedes is said to have taken an immersion bath and observed from the rise of the water upon entering that he could calculate the volume of the gold wreath through the displacement of the water. Upon this discovery, he leapt from his bath and ran naked through the streets shouting, "Eureka! Eureka!" (Ancient Greek: Εύρηκα!, lit.'I have found it'). As a result, the term eureka entered common parlance and is used today to indicate a moment of enlightenment.

The story first appeared in written form in Vitruvius' books of architecture, two centuries after it supposedly took place.[7] Some scholars have doubted the accuracy of this tale, saying among other things that the method would have required precise measurements that would have been difficult to make at the time.[8][9]

Nevertheless, in 1586, Galileo Galilei, in one of his first experiments, made a possible reconstruction of how the experiment could have been performed with ancient Greek resources.[10]

Units

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From the equation for density (ρ = m/V), mass density has any unit that is mass divided by volume. As there are many units of mass and volume covering many different magnitudes there are a large number of units for mass density in use. The SI unit of kilogram per cubic metre (kg/m3) and the cgs unit of gram per cubic centimetre (g/cm3) are probably the most commonly used units for density. In industry, other larger or smaller units of mass and or volume are often more practical and US customary units may be used. See below for a list of some of the most common units of density.

Densities using the following metric units all have exactly the same numerical value, one-thousandth of the value in kg/m3. Liquid water has a density of about 1 g/cm3 or 1000 kg/m3, making any of these SI units numerically convenient to use as most solids and liquids have densities between 0.1 and 20 g/cm3.

The litre and tonne (metric ton) are not part of the SI, but are accepted for use with it, leading to the following equivalent metric units:

In US customary units density can be stated in:

Imperial units differing from the above (as the Imperial gallon and bushel differ from the US units) in practice are rarely used, though found in older documents. The Imperial gallon was based on the concept that an Imperial fluid ounce of water would have a mass of one Avoirdupois ounce, and indeed 1 g/cm3 ≈ 1.00224129 ounces per Imperial fluid ounce = 10.0224129 pounds per Imperial gallon. The density of precious metals could conceivably be based on Troy ounces and pounds, a possible cause of confusion.

The density of a crystalline material and be calculated from its formula mass (in daltons) and the volume of its unit cell, the density can be calculated. One dalton per cubic ångström is equal to a density of 1.66053906892(52) g/cm3, based on the 2022 CODATA recommended value of the dalton.[11]

Measurement

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A number of techniques as well as standards exist for the measurement of density of materials. Such techniques include the use of a hydrometer (a buoyancy method for liquids), Hydrostatic balance (a buoyancy method for liquids and solids), immersed body method (a buoyancy method for liquids), pycnometer (liquids and solids), air comparison pycnometer (solids), oscillating densitometer (liquids), as well as pour and tap (solids).[12] However, each individual method or technique measures different types of density (e.g. bulk density, skeletal density, etc.), and therefore it is necessary to have an understanding of the type of density being measured as well as the type of material in question.

Homogeneous materials

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The density at all points of a homogeneous object equals its total mass divided by its total volume. The mass is normally measured with a scale or balance; the volume may be measured directly (from the geometry of the object) or by the displacement of a fluid. To determine the density of a liquid or a gas, a hydrometer, a dasymeter or a Coriolis flow meter may be used, respectively. Similarly, hydrostatic weighing uses the displacement of water due to a submerged object to determine the density of the object.

Heterogeneous materials

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If the body is not homogeneous, then its density varies between different regions of the object. In that case the density around any given location is determined by calculating the density of a small volume around that location. In the limit of an infinitesimal volume the density of an inhomogeneous object at a point becomes: , where is an elementary volume at position . The mass of the body then can be expressed as

Non-compact materials

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In practice, bulk materials such as sugar, sand, or snow contain voids. Many materials exist in nature as flakes, pellets, or granules.

Voids are regions which contain something other than the considered material. Commonly the void is air, but it could also be vacuum, liquid, solid, or a different gas or gaseous mixture.

The bulk volume of a material—inclusive of the void space fraction—is often obtained by a simple measurement (e.g. with a calibrated measuring cup) or geometrically from known dimensions.

Mass divided by bulk volume determines bulk density. This is not the same thing as the material volumetric mass density. To determine the material volumetric mass density, one must first discount the volume of the void fraction. Sometimes this can be determined by geometrical reasoning. For the close-packing of equal spheres the non-void fraction can be at most about 74%. It can also be determined empirically. Some bulk materials, however, such as sand, have a variable void fraction which depends on how the material is agitated or poured. It might be loose or compact, with more or less air space depending on handling.

In practice, the void fraction is not necessarily air, or even gaseous. In the case of sand, it could be water, which can be advantageous for measurement as the void fraction for sand saturated in water—once any air bubbles are thoroughly driven out—is potentially more consistent than dry sand measured with an air void.

In the case of non-compact materials, one must also take care in determining the mass of the material sample. If the material is under pressure (commonly ambient air pressure at the earth's surface) the determination of mass from a measured sample weight might need to account for buoyancy effects due to the density of the void constituent, depending on how the measurement was conducted. In the case of dry sand, sand is so much denser than air that the buoyancy effect is commonly neglected (less than one part in one thousand).

Mass change upon displacing one void material with another while maintaining constant volume can be used to estimate the void fraction, if the difference in density of the two voids materials is reliably known.

Changes of density

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In general, density can be changed by changing either the pressure or the temperature. Increasing the pressure always increases the density of a material. Increasing the temperature generally decreases the density, but there are notable exceptions to this generalization. For example, the density of water increases between its melting point at 0 °C and 4 °C; similar behavior is observed in silicon at low temperatures.

The effect of pressure and temperature on the densities of liquids and solids is small. The compressibility for a typical liquid or solid is 10−6 bar−1 (1 bar = 0.1 MPa) and a typical thermal expansivity is 10−5 K−1. This roughly translates into needing around ten thousand times atmospheric pressure to reduce the volume of a substance by one percent. (Although the pressures needed may be around a thousand times smaller for sandy soil and some clays.) A one percent expansion of volume typically requires a temperature increase on the order of thousands of degrees Celsius.

In contrast, the density of gases is strongly affected by pressure. The density of an ideal gas is where M is the molar mass, P is the pressure, R is the universal gas constant, and T is the absolute temperature. This means that the density of an ideal gas can be doubled by doubling the pressure, or by halving the absolute temperature.

In the case of volumic thermal expansion at constant pressure and small intervals of temperature the temperature dependence of density is where is the density at a reference temperature, is the thermal expansion coefficient of the material at temperatures close to .

Density of solutions

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The density of a solution is the sum of mass (massic) concentrations of the components of that solution.

Mass (massic) concentration of each given component in a solution sums to density of the solution,

Expressed as a function of the densities of pure components of the mixture and their volume participation, it allows the determination of excess molar volumes: provided that there is no interaction between the components.

Knowing the relation between excess volumes and activity coefficients of the components, one can determine the activity coefficients:

List of densities

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Various materials

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Densities of various materials covering a range of values
Material ρ (kg/m3)[note 1] Notes
Hydrogen 0.0898
Helium 0.179
Aerographite 0.2 [note 2][13][14]
Metallic microlattice 0.9 [note 2]
Aerogel 1.0 [note 2]
Air 1.2 At sea level
Tungsten hexafluoride 12.4 One of the heaviest known gases at standard conditions
Liquid hydrogen 70 At approximately −255 °C
Styrofoam 75 Approximate[15]
Cork 240 Approximate[15]
Pine 373 [16]
Lithium 535 Least dense metal
Wood 700 Seasoned, typical[17][18]
Oak 710 [16]
Potassium 860 [19]
Ice 916.7 At temperature < 0 °C
Cooking oil 910–930
Sodium 970
Water (fresh) 1,000 Maximum, occurs at approximately 4 °C
Water (salt) 1,030 Salinity of 3%
Liquid oxygen 1,141 At approximately −219 °C
Nylon 1,150
Plastics 1,175 Approximate; for polypropylene and PETE/PVC
Glycerol 1,261 [20]
Tetrachloroethene 1,622
Sand 1,600 Between 1,600 and 2,000 [21]
Magnesium 1,740
Beryllium 1,850
Silicon 2,330
Concrete 2,400 [22][23]
Glass 2,500 [24]
Quartzite 2,600 [21]
Granite 2,700 [21]
Gneiss 2,700 [21]
Aluminium 2,700
Limestone 2,750 Compact[21]
Basalt 3,000 [21]
Diiodomethane 3,325 Liquid at room temperature
Diamond 3,500
Titanium 4,540
Selenium 4,800
Vanadium 6,100
Antimony 6,690
Zinc 7,000
Chromium 7,200
Tin 7,310
Manganese 7,325 Approximate
Mild steel 7,850
Iron 7,870
Niobium 8,570
Brass 8,600 [23]
Cadmium 8,650
Cobalt 8,900
Nickel 8,900
Copper 8,940
Bismuth 9,750
Molybdenum 10,220
Silver 10,500
Lead 11,340
Thorium 11,700
Rhodium 12,410
Mercury 13,546
Tantalum 16,600
Uranium 19,100
Tungsten 19,300
Gold 19,320
Plutonium 19,840
Rhenium 21,020
Platinum 21,450
Iridium 22,420
Osmium 22,570 Densest natural element on Earth
  1. ^ Unless otherwise noted, all densities given are at standard conditions for temperature and pressure,
    that is, 273.15 K (0.00 °C) and 100 kPa (0.987 atm).
  2. ^ a b c Air contained in material excluded when calculating density

Others

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Entity ρ (kg/m3) Notes
Interstellar medium 1.7×10−26 Based on 10−5 hydrogen atoms per cubic centimetre[25]
Local Interstellar Cloud 5×10−22 Based on 0.3 hydrogen atoms per cubic centimetre[25]
Interstellar medium 1.7×10−16 Based on 105 hydrogen atoms per cubic centimetre[25]
The Earth 5,515 Mean density.[26]
Earth's inner core 13,000 Approx., as listed in Earth.[27]
The core of the Sun 33,000–160,000 Approx.[28]
White dwarf star 2.1×109 Approx.[29]
Atomic nuclei 2.3×1017 Does not depend strongly on size of nucleus[30]
Neutron star 1×1018

Water

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Density of liquid water at 1 atm pressure
Temp. (°C)[note 1] Density (kg/m3)
−30 983
.854
−20 993
.547
−10 998
.117
0 999
.8395
4 999
.9720
10 999
.7026
15 999
.1026
20 998
.2071
22 997
.7735
25 997
.0479
30 995
.6502
40 992
.2
60 983
.2
80 971
.8
100 958
.4

Notes:

  1. ^ Values below 0 °C refer to supercooled water.

Air

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Air density vs. temperature
Density of air at 1 atm pressure
T (°C) ρ (kg/m3)
−25 1.423
−20 1.395
−15 1.368
−10 1.342
−5 1.316
0 1.293
5 1.269
10 1.247
15 1.225
20 1.204
25 1.184
30 1.164
35 1.146

Molar volumes of liquid and solid phase of elements

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Molar volumes of liquid and solid phase of elements

Generalization: volumic quantities

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The qualifier volumic is recommended in the International System of Quantities (ISO 80000-1) to denote the quotient of any physical quantity by volume.[3] The expressions "per unit volume" or "volume ... density" (or simply "density") are also often used, with resulting units involving reciprocal cubic metre (m−3), for example:

See also

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References

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[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Density is a fundamental of that quantifies the of a substance per unit , serving as a measure of how compact or concentrated the material is. It is mathematically expressed by the formula ρ = m / V, where ρ (the Greek letter rho) represents density, m is the , and V is the . The SI unit of density is kilograms per cubic meter (kg/m³), though other common units include grams per cubic centimeter (g/cm³) for solids and liquids. As an intensive property, density remains constant for a given substance regardless of the sample , distinguishing it from extensive properties like or that scale with . This characteristic makes density invaluable for identifying and characterizing materials, such as distinguishing metals like lead (density ≈ 11.34 g/cm³) from lighter substances like aluminum (density ≈ 2.70 g/cm³). In fluids, density plays a critical role in phenomena like , where objects denser than the surrounding fluid sink, while less dense ones float, as explained by . Density varies with and , particularly for gases and liquids, due to changes in volume while mass remains constant; for instance, most substances expand when heated, decreasing their density. In scientific applications, density measurements enable quality control in industries like and pharmaceuticals—for example, assessing alcohol content in beverages or purity in oils—and support , such as tracking through density gradients. It also informs designs, from to ensure flotation to in for structural integrity.

Definition and Fundamentals

Core Definition

Density, denoted by the Greek letter ρ, is the mm of a substance divided by its VV, expressed as ρ=mV.\rho = \frac{m}{V}. This quantity, known as mass density, characterizes how compactly the matter in a substance is packed. Mass density is distinct from other types of density, such as (the number of particles per unit volume) or (the per unit volume), which apply to specific contexts in physics like or . As an intensive , density remains constant regardless of the sample size or ; for example, a small or a large block of the same material will exhibit the same density value under identical conditions. In everyday scenarios, density determines whether objects sink or float in fluids: lead sinks in due to its higher density, while floats because of its lower density relative to . This principle underlies effects observed in fluids.

Mathematical Formulation

The mass density ρ\rho of is fundamentally defined as the ratio of to in the limit as the approaches zero, ensuring a pointwise characterization suitable for continuous media. Specifically, for a point at position r\mathbf{r}, the density is given by ρ(r)=limΔV0ΔmΔV\rho(\mathbf{r}) = \lim_{\Delta V \to 0} \frac{\Delta m}{\Delta V}, where Δm\Delta m is the contained within an infinitesimal ΔV\Delta V surrounding r\mathbf{r}. This limiting process arises from the in , which posits that matter can be modeled as a continuous distribution despite its atomic structure, allowing density to capture local concentration without regard to microscopic discreteness. For materials with non-uniform distribution, density extends to a position-dependent function ρ(r)\rho(\mathbf{r}), representing the local value at each point r\mathbf{r} via the same limit: ρ(r)=limΔV0ΔmΔV\rho(\mathbf{r}) = \lim_{\Delta V \to 0} \frac{\Delta m}{\Delta V} as ΔV\Delta V shrinks around r\mathbf{r}. In , this local density is treated as a ρ:R3R\rho: \mathbb{R}^3 \to \mathbb{R}, varying continuously across the domain to describe heterogeneous distributions. The total mm of a body occupying volume VV is then obtained by integrating this field: m=Vρ(r)dV,m = \int_V \rho(\mathbf{r}) \, dV, which follows directly from the additivity of over disjoint subvolumes and the definition of the as a limit of sums. In the framework of , density acquires additional complexity due to spacetime , manifesting as components of the stress-energy tensor TμνT_{\mu\nu}. Here, proper density refers to the invariant measured in the local of the , while coordinate density denotes the value in a specific , which transforms non-trivially under changes of coordinates. This distinction underscores the tensorial nature of density in curved spacetime, where it contributes to the geometry via Einstein's field equations without altering the core limit-based definition.

Historical Development

Early Observations and Concepts

Early observations of density-like phenomena emerged from intuitive understandings of why objects sink or float in , laying the groundwork for more formalized concepts. In ancient civilizations, such as and , practical knowledge of material weights relative to volume informed construction and metallurgy, though these were not systematically theorized. The ancient advanced this into philosophical and empirical , distinguishing between concepts akin to modern density and mere weight. Aristotle (384–322 BCE) conceptualized natural elements as having inherent "light" or "heavy" properties that determined their tendency to move upward or downward in a medium like air or water. In his work On the Heavens, he described lighter elements like fire and air as rising, while heavier ones like earth and water sank, attributing this to their natural places in the cosmos rather than a quantitative ratio of mass to volume. This qualitative framework influenced Western thought for centuries, emphasizing elemental affinities over precise measurement. A pivotal empirical breakthrough occurred with (c. 287–212 BCE), who linked to the displacement of fluid, providing an early method to assess density. Legendarily, while tasked by King Hieron II to verify if was pure or adulterated, Archimedes realized in his bath that the volume of displaced water equaled the object's submerged volume, allowing density calculation as mass divided by volume without damaging the crown—famously exclaiming "Eureka!" This principle, detailed in his , established that an object's density relative to the fluid determines flotation, forming the basis of . During the medieval period, these ideas persisted in and Islamic scholarship, where scholars like (c. 1115–1130) explored balances for comparing material densities in works like The Book of the Balance of Wisdom, integrating Greek principles with experimental refinements. In the , (1564–1642) built on in (1638), analyzing why bodies of the same material but different float differently, emphasizing and shape over intrinsic heaviness alone. The transition to quantitative density occurred with (1643–1727), who in (1687) treated density as the ratio of to , using it to describe gravitational attraction and fluid equilibrium. Newton's formulation, such as in Proposition 19 of Book II, applied density to explain hydrostatic pressure variations, shifting from qualitative to mathematical rigor. This marked the evolution from observational concepts to a foundational .

Evolution of Measurement Techniques

During the , the Enlightenment era marked a pivotal shift toward quantitative precision in scientific measurements, including density, through refinements in balances and volumetric devices. , leveraging advanced analytical balances, conducted meticulous determinations that facilitated accurate density computations when integrated with displacement or volumetric techniques, emphasizing the balance's role in establishing conservation laws in chemistry. Lavoisier further contributed by improving designs, such as those used to assess the density of mineral waters, thereby enhancing the reliability of evaluations for liquids. These instruments, often hydrostatic balances adapted for buoyancy-based measurements, allowed chemists to control for purity in metals and solutions with greater accuracy than previous qualitative methods. The 19th century brought further innovations, particularly in s and specialized apparatus for both liquids and solids. William Nicholson's constant-volume , introduced in 1784 but widely adopted and refined in the early 1800s, enabled precise specific gravity measurements for liquids and by maintaining a fixed displaced while varying weights. For liquids, Henri Victor Regnault's pycnometers, designed in 1843, represented a breakthrough with their calibrated flasks that minimized errors from and fluctuations, achieving densities with uncertainties below 0.1%. Regarding solids, oscillation-based methods emerged toward the century's end, such as those involving torsional pendulums or vibrating systems to infer density from resonant frequencies in fluids, though via spring balances like Philipp von Jolly's 1881 apparatus became standard for routine specific gravity assessments without destructive sampling. The introduced non-invasive and microscopic techniques, expanding density measurements beyond macroscopic samples. , developed by and his son William Lawrence Bragg starting in 1912, permitted atomic-level density calculations by determining volumes and atomic arrangements; early applications in the 1920s, such as for , yielded theoretical densities matching experimental values within 1%, revolutionizing solid-state analysis. Ultrasound methods for non-destructive testing gained traction from the 1940s, using pulse-echo propagation to measure acoustic velocities in materials like metals and composites, from which bulk densities could be derived via empirical correlations with wave attenuation and impedance, offering in-situ assessments without material alteration. In contemporary practice, computational approaches have complemented experimental methods, particularly through (DFT) in . The foundational Hohenberg-Kohn theorems of 1964 established that the ground-state uniquely determines all molecular properties, enabling DFT algorithms to predict material densities ab initio; for instance, calculations for semiconductors and polymers now achieve accuracies rivaling measurements, with errors often under 5% for bulk moduli and densities.

Units and Standards

Common Units and Systems

The (SI) defines density as per unit volume, with the standard unit being the per cubic meter (kg/m³), derived from the base units of (, kg) and length (meter, m), where volume is expressed as cubic meters (m³). This unit is universally adopted in scientific and international contexts for its coherence with other SI-derived quantities. In Imperial and customary systems, density is commonly expressed in pounds per (lb/ft³), where the pound (lb) represents , though slugs per (slug/ft³) is used in contexts requiring consistency with force units like the pound-force (lbf). These units have historical prevalence in engineering applications, particularly in the and , for structural and calculations predating widespread metric adoption. Other frequently used units include grams per cubic centimeter (g/cm³), which is convenient for measuring the density of and liquids due to its alignment with typical scales. For dilute aqueous solutions, such as in environmental or chemical , milligrams per liter (mg/L) serves as a practical unit, approximating mass concentration where the solution's volume is close to that of the . In , density has the formula [M L⁻³], where M denotes and L denotes , reflecting its role as mass distributed over . This dimension connects density to derived quantities like ([M L T⁻²]) through relations such as weight (force equals times ) and ([M L⁻¹ T⁻²]), as seen in hydrostatic equations where depends on density, , and depth.
System/UnitUnit SymbolTypical Application
SIkg/m³General scientific and engineering use
Imperial/US Customarylb/ft³ or slug/ft³,
CGS/Metricg/cm³Solids and liquids in laboratories
Environmental/Chemicalmg/LDilute solutions and concentrations
, or specific gravity, is a dimensionless comparing a substance's density to a reference (often ), avoiding unit dependencies.

Conversions and Relative Density

Density units can be converted between different systems using , a method that ensures consistency by treating units as algebraic quantities. For instance, to convert from grams per cubic centimeter (g/cm³) to kilograms per cubic meter (kg/m³), multiply the value by the factor 1000, derived from the relations 1 kg = 1000 g and 1 m³ = 10^6 cm³, yielding 1 g/cm³ = 1000 kg/m³. This approach applies broadly: identify the conversion factors for and separately, then combine them to cancel undesired units step by step. Relative density, also known as specific gravity, is defined as the unitless ratio of the density of a substance to the density of a reference substance under specified conditions. For liquids and solids, the reference is typically at , where its density is maximized at approximately 1000 kg/m³; for gases, the reference is dry air at . This ratio, denoted as SG, is expressed mathematically as SG=ρρreference\text{SG} = \frac{\rho}{\rho_\text{reference}} where ρ\rho is the density of the substance and ρreference\rho_\text{reference} is the density of the reference material, often (\rho_\text{H_2O}) for liquids. The concept of specific gravity has historical roots in chemistry, notably through the developed by French chemist Antoine Baumé in 1768, which used hydrometers to measure relative densities of liquids for industrial applications like and acid production. This scale provided two versions—one for liquids denser than and one for those less dense—calibrated against specific gravity to simplify comparisons without needing absolute density values. The primary advantage of relative density lies in its unitless nature, enabling direct, standardized comparisons of material properties across substances and conditions, independent of the unit system used for absolute density. However, specific gravity values are temperature-dependent, as both the substance's density and the reference density vary with ; thus, measurements must specify the temperature to ensure accuracy and comparability.

Measurement Methods

For Homogeneous Solids and Liquids

For homogeneous solids, density is commonly measured using , which relies on the buoyant force experienced by an object submerged in a . The principle states that the buoyant force FbF_b equals the weight of the displaced by the object, given by Fb=ρfVgF_b = \rho_f V g, where ρf\rho_f is the density, VV is the of the displaced (equal to the object's for full submersion), and gg is the acceleration due to gravity. To apply this, the solid is weighed in air (Wair=mgW_{\text{air}} = m g, where mm is the ) and then submerged in a of known density, such as , to obtain the WfluidW_{\text{fluid}}. The is calculated as V=WairWfluidρfgV = \frac{W_{\text{air}} - W_{\text{fluid}}}{\rho_f g}, and the density follows as ρ=mV=WairρfWairWfluid\rho = \frac{m}{V} = \frac{W_{\text{air}} \rho_f}{W_{\text{air}} - W_{\text{fluid}}}. This method is particularly suitable for regular-shaped homogeneous solids like metal cubes or cylinders, as it directly determines without needing geometric measurements. Modern implementations often use analytical balances for precise weighing, achieving accuracies on the order of 0.1% for densities around 1–10 g/cm³. For liquids, pycnometry provides a standard volumetric technique by employing a pycnometer—a flask of precisely known , typically calibrated with . The process involves weighing the empty pycnometer (memptym_{\text{empty}}), filling it completely with the sample and weighing again (mliquidm_{\text{liquid}}), and sometimes accounting for the flask's calibration using a reference . The density is then computed as ρ=mliquidmemptyVflask\rho = \frac{m_{\text{liquid}} - m_{\text{empty}}}{V_{\text{flask}}}, where VflaskV_{\text{flask}} is the internal at a specified . This method ensures high precision for homogeneous liquids like oils or solvents, as the pycnometer's design minimizes air bubbles and evaporation errors. standards, such as those from the International Union of Pure and Applied Chemistry (IUPAC), recommend using deionized at 20°C for determination, yielding results traceable to SI units. Typical laboratory pycnometers achieve resolutions better than 0.001 g/cm³ for volumes around 10–50 mL. A more advanced approach for both solids (via immersion) and liquids is the digital density meter, which utilizes the oscillating U-tube principle invented in the by researchers at the company. In this device, a U-shaped tube filled with the sample vibrates at its , where the period TT is proportional to the of the sample's density: TρT \propto \sqrt{\rho}
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