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Specific volume
Specific volume
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In thermodynamics, the specific volume of a substance (symbol: ν, nu) is the quotient of the substance's volume (V) to its mass (m):

It is a mass-specific intrinsic property of the substance. It is the reciprocal of density ρ (rho) and it is also related to the molar volume and molar mass:

The standard unit of specific volume is cubic meters per kilogram (m3/kg), but other units include ft3/lb, ft3/slug, or mL/g.[1]

Specific volume for an ideal gas is related to the molar gas constant (R) and the gas's temperature (T), pressure (P), and molar mass (M) as shown:

Since and

Applications

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Specific volume is commonly applied to:

Imagine a variable-volume, airtight chamber containing a certain number of atoms of oxygen gas. Consider the following four examples:

  • If the chamber is made smaller without allowing gas in or out, the density increases and the specific volume decreases.
  • If the chamber expands without letting gas in or out, the density decreases and the specific volume increases.
  • If the size of the chamber remains constant and new atoms of gas are injected, the density increases and the specific volume decreases.
  • If the size of the chamber remains constant and some atoms are removed, the density decreases and the specific volume increases.

Specific volume is a property of materials, defined as the number of cubic meters occupied by one kilogram of a particular substance. The standard unit is the meter cubed per kilogram (m3/kg or m3·kg−1).

Sometimes specific volume is expressed in terms of the number of cubic centimeters occupied by one gram of a substance. In this case, the unit is the centimeter cubed per gram (cm3/g or cm3·g−1). To convert m3/kg to cm3/g, multiply by 1000; conversely, multiply by 0.001.

Specific volume is inversely proportional to density. If the density of a substance doubles, its specific volume, as expressed in the same base units, is cut in half. If the density drops to 1/10 its former value, the specific volume, as expressed in the same base units, increases by a factor of 10.

The density of gases changes with even slight variations in temperature, while densities of liquid and solids, which are generally thought of as incompressible, will change very little. Specific volume is the inverse of the density of a substance; therefore, careful consideration must be taken account when dealing with situations that involve gases. Small changes in temperature will have a noticeable effect on specific volumes.

The average density of human blood is 1060 kg/m3. The specific volume that correlates to that density is 0.00094 m3/kg. Notice that the average specific volume of blood is almost identical to that of water: 0.00100 m3/kg.[2]

Application examples

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If one sets out to determine the specific volume of an ideal gas, such as super heated steam, using the equation ν = RT/P, where pressure is 2500 lbf/in2, R is 0.596, temperature is 1960 °R. In that case, the specific volume would equal 0.4672 in3/lb. However, if the temperature is changed to 1160 °R, the specific volume of the super heated steam would have changed to 0.2765 in3/lb, which is a 59% overall change.

Knowing the specific volumes of two or more substances allows one to find useful information for certain applications. For a substance X with a specific volume of 0.657 cm3/g and a substance Y with a specific volume 0.374 cm3/g, the density of each substance can be found by taking the inverse of the specific volume; therefore, substance X has a density of 1.522 g/cm3 and substance Y has a density of 2.673 g/cm3. With this information, the specific gravities of each substance relative to one another can be found. The specific gravity of substance X with respect to Y is 0.569, while the specific gravity of Y with respect to X is 1.756. Therefore, substance X will not sink if placed on Y.[3]

Specific volume of solutions

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The specific volume of a non-ideal solution is the sum of the partial specific volumes of the components:

M is the molar mass of the mixture. This can be used instead of volume, as this is intensive property tied to the system.

Table of common specific volumes

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The table below displays densities and specific volumes for various common substances that may be useful. The values were recorded at standard temperature and pressure, which is defined as air at 0 °C (273.15 K, 32 °F) and 1 atm (101.325 kN/m2, 101.325 kPa, 14.7 psia, 0 psig, 30 in Hg, 760 torr).[4]

Substance name Density Specific volume[dubiousdiscuss]
(kg/m3) (m3/kg)
Air 1.225 0.816
Ice 916.7 0.00109
Water (liquid) 1000 0.00100
Salt Water 1030 0.00097
Mercury 13546 0.00007
R-22* 3.66 0.273
Ammonia 0.769 1.30
Carbon dioxide 1.977 0.506
Chlorine 2.994 0.334
Hydrogen 0.0899 11.12
Methane 0.717 1.39
Nitrogen 1.25 0.799
Steam* 0.804 1.24

* values not taken at standard temperature and pressure

References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Specific volume is a fundamental thermodynamic property defined as the volume occupied by a unit mass of a substance, expressed as v=Vmv = \frac{V}{m}, where VV is the total volume and mm is the mass, with typical units of cubic meters per kilogram (m³/kg). As an intensive property, specific volume remains independent of the system's size and is crucial for determining the thermodynamic state of a substance, often alongside or . It is the reciprocal of (v=1ρv = \frac{1}{\rho}, where ρ\rho is mass per unit volume), providing a measure of how compact or expansive a is under given conditions. In practical applications, specific volume is essential for analyzing gas behavior via the (Pv=RTPv = RT, where PP is , RR is the specific , and TT is ), enabling calculations in processes like compression, expansion, and in systems. For two-phase mixtures, such as liquid-vapor systems, it is computed as a quality-weighted : v=(1x)vf+xvgv = (1 - x) v_f + x v_g, where xx is the , vfv_f is the saturated liquid specific volume, and vgv_g is the saturated vapor specific volume, which is vital for phase change analyses in steam tables and cycles.

Fundamentals

Definition

Specific volume, denoted as vv, is defined as the ratio of the volume VV of a substance to its mass mm, mathematically expressed as v=Vmv = \frac{V}{m}. This quantity provides a measure of the space occupied by a unit mass of the material under given conditions. Physically, specific volume represents the volumetric extent per unit mass, which is essential for analyzing how substances expand or contract in response to changes in their state, such as during heating or compression. Unlike extensive properties like total volume, which scale with the size of the system, specific volume is an intensive property, remaining constant regardless of the amount of substance considered. The concept of specific volume emerged in the 19th century within the developing field of thermodynamics, where it helped standardize measurements of volume in engineering analyses, particularly for heat engines and gas behavior. Early uses appear in works like Clapeyron's 1834 diagrams for thermodynamic cycles and later in van der Waals' 1873 equation for real gases, reflecting its role in precise property characterization.

Units and Notation

The SI unit for specific volume is the cubic meter per kilogram (m³/kg), derived from the base units of volume (cubic meter) and mass (). In engineering contexts, common alternative units include the cubic foot per pound (ft³/lb) in customary systems and liters per gram (L/g) or cubic centimeters per gram (cm³/g) for smaller-scale measurements. Specific volume is typically denoted by the lowercase letter vv, representing the volume per unit mass. The molar specific volume, which is the volume per unit amount of substance, is denoted by vˉ=V/n\bar{v} = V/n, where VV is the total volume and nn is the number of moles./03%3A_Conservation_of_Mass/3.06%3A_Density_Specific_Volume_Specific_Weight_and_Specific_Gravity) Conversion between units is straightforward using standard factors, as specific volume scales inversely with units. The following table provides key conversion factors to and from the SI unit:
UnitAbbreviationConversion Factor to m³/kg
per poundft³/lb1 ft³/lb = 0.06243 m³/kg
Liter per gramL/g1 L/g = 1 m³/kg
Cubic centimeter per gramcm³/g1 cm³/g = 0.001 m³/kg
These conversions are based on the relations 1 lb ≈ 0.4536 kg, 1 ft³ ≈ 0.02832 m³, 1 L = 0.001 m³, and 1 g = 0.001 kg. Specific volume is measured by determining the ratio of to , with methods varying by phase. For liquids and , volumetric displacement techniques are standard, such as using a pycnometer—a flask of known filled with the sample and weighed to find —or the for irregular by submerging in a to measure displaced . For gases, pressure- relations are employed, typically by confining the gas in a calibrated container of known , measuring the and , and determining via weighing or other means, often under controlled conditions to account for .

Relations to Other Properties

Relation to Density

Specific volume, denoted as vv, is defined as the volume per unit mass of a substance, v=V/mv = V / m, where VV is the total and mm is the . , denoted as ρ\rho, is the mass per unit , ρ=m/V\rho = m / V. Substituting the expression for vv into the density formula yields the direct mathematical relation ρ=1/v\rho = 1 / v, demonstrating that specific volume and are reciprocals of each other. This inverse relationship arises fundamentally from the definitions, as an increase in for a fixed decreases while increasing specific volume. The reciprocal nature has practical implications in characterizing material states: specific volume emphasizes the "sparsity" or openness of a substance's structure, particularly useful for gases where vv is large (e.g., air at standard conditions has v0.8m3/kgv \approx 0.8 \, \mathrm{m}^3/\mathrm{kg}), corresponding to low , whereas density highlights compactness, which is more intuitive for dense liquids and solids. For instance, this distinction aids in comparing phases, as gases exhibit high specific volumes and low densities due to greater intermolecular spacing, while liquids show the opposite. Specific volume also connects to compressibility through its partial derivative with respect to pressure. The isothermal compressibility , which quantifies volume change under constant temperature, is defined as κT=1v(vP)T\kappa_T = -\frac{1}{v} \left( \frac{\partial v}{\partial P} \right)_T. This expression links the rate of change of specific volume to the substance's resistance to compression, with the negative sign indicating volume decrease under increasing . As an example, for liquid at (0°C and 1 atm), the specific volume is approximately v0.001m3/kgv \approx 0.001 \, \mathrm{m}^3/\mathrm{kg}, yielding a of ρ=1/v1000kg/m3\rho = 1 / v \approx 1000 \, \mathrm{kg}/\mathrm{m}^3. This calculation illustrates the inverse relation in a common fluid, where small changes in vv correspond to significant shifts in ρ\rho.

Temperature and Pressure Effects

The specific volume of a substance varies with at constant primarily through , quantified by the volumetric thermal expansion coefficient α=1v(vT)P\alpha = \frac{1}{v} \left( \frac{\partial v}{\partial T} \right)_P, where vv is the specific volume and TT is the . For small temperature changes ΔT\Delta T, this leads to the approximate relation v(T)v0(1+αΔT)v(T) \approx v_0 (1 + \alpha \Delta T), where v0v_0 is the initial specific volume. This effect arises because increased causes particles to vibrate more intensely, increasing intermolecular distances and thus the volume per unit mass. The magnitude of thermal expansion differs markedly across states of matter. Gases exhibit significant expansion with rising at constant pressure, as their low allows substantial intermolecular separation; for instance, under near-ideal conditions, specific volume is directly proportional to via . Liquids show a moderate increase in specific volume, with α\alpha values typically on the order of 10310^{-3} to 10410^{-4} K1^{-1}, reflecting constrained molecular motion compared to gases. Solids, by contrast, display negligible changes, with α3×105\alpha \approx 3 \times 10^{-5} K1^{-1} or smaller, due to strong interatomic bonds that limit expansion. Pressure influences specific volume at constant temperature through compressibility, defined by the isothermal compressibility κT=1v(vP)T\kappa_T = -\frac{1}{v} \left( \frac{\partial v}{\partial P} \right)_T, where PP is pressure. For gases behaving nearly ideally, specific volume decreases inversely with pressure (v1/Pv \propto 1/P), as molecules are forced closer together, enabling large volume reductions even at moderate pressures. In liquids, however, low compressibility (κT\kappa_T on the order of 10910^{-9} to 101010^{-10} Pa1^{-1}) results in minimal specific volume changes, requiring extreme pressures to achieve noticeable compression. Solids exhibit even lower compressibility, with volume reductions that are practically insignificant under typical conditions. These dependencies are often visualized in pressure-volume-temperature (PVT) diagrams, where isotherms (constant lines) show specific volume decreasing with , particularly steeply for gases, and isobars (constant lines) illustrate volume increasing with , with the steepest slopes for gases. Such representations highlight the contrasting behaviors: gases occupy a broad region with hyperbolic isotherms and linear isobars, while liquids and solids cluster near constant volume, underscoring their relative incompressibility and limited .

Thermodynamic Contexts

Equations of State

Equations of state provide mathematical relations that connect specific volume to other thermodynamic properties such as , , and mass for substances, particularly gases. These equations are essential for predicting the behavior of fluids under varying conditions, enabling calculations in and scientific applications. For ideal gases, the simplest form assumes no intermolecular forces or molecular volume, leading to a direct proportionality between specific volume and at constant . The , derived from the universal gas law PV=nRuTPV = n R_u T, where PP is , VV is total volume, nn is the number of moles, RuR_u is the universal , and TT is , can be expressed in terms of specific volume v=V/mv = V/m by substituting n=m/Mn = m/M (with mm as mass and MM as ). This yields Pv=RTP v = R T, where R=Ru/MR = R_u / M is the specific for the substance. This relation holds well for gases at low pressures and high temperatures where deviations from ideality are negligible. Real gases deviate from ideal behavior due to intermolecular attractions and the finite volume of molecules, necessitating corrections to the . The accounts for these by modifying and volume terms: (P+av2)(vb)=RT\left( P + \frac{a}{v^2} \right) (v - b) = R T, where aa corrects for attractive forces reducing effective , and bb accounts for the per unit (with aa and bb as mass-specific constants, related to molar constants by a=au/M2a = a_u / M^2, b=bu/Mb = b_u / M). This equation better predicts and phase behavior for gases near . For instance, at high densities, the a/v2a/v^2 term becomes significant, reducing the predicted specific volume compared to the ideal case. Other equations of state extend these corrections for specific applications. The Redlich-Kwong equation, developed for hydrocarbons, improves upon van der Waals by introducing temperature dependence in the attraction term: P=RTvbaTv(v+b)P = \frac{R T}{v - b} - \frac{a}{\sqrt{T} v (v + b)}
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