4.3 - Density and pressure in fluids

4.3 - Density and pressure in fluids

Calculate density from mass and geometry, relate pressure to the normal force on an area, and derive the pressure difference between two depths in a fluid. Use the vertical depth and distinguish extra pressure due to a liquid from the total pressure.

Mass per unit volume

Would a narrow tube of water give less pressure at its bottom than a wide tank of water at the same depth? The tank contains much more water, but that alone does not settle the question. First distinguish how much material there is from how closely its mass is packed.

Density compares mass with volume. Two objects made of the same homogeneous material at the same temperature have the same density even when their masses and volumes differ.

Density

Density is mass per unit volume.

If 0.010 m30.010\,\mathrm{m^{3}} of a material has mass 27 kg27\,\mathrm{kg}, each cubic metre would have mass 2700 kg2700\,\mathrm{kg} for the same homogeneous material. That is the meaning of the density, rather than a claim that the particular sample contains a cubic metre.

Density

ρ=mV\rho=\frac{m}{V}

Here ρ\rho is density in kg m−3\mathrm{kg\,m^{-3}}, mm is mass in kg\mathrm{kg}, and VV is volume in m3\mathrm{m^{3}}. Use the volume of the material whose density you want. A whole object's average density can include its internal empty space; its material density does not.

Not on the data sheet: learn it.

Geometry gives the volume

Convert lengths before squaring or cubing. Use the radius, half the diameter, in circle, cylinder and sphere formulae. For the following shapes, all lengths are in m\mathrm{m}; area and surface area are in m2\mathrm{m^{2}}, perimeter or circumference in m\mathrm{m}, and volume in m3\mathrm{m^{3}}.

Plane shapeAreaPerimeter or circumference
Rectangle, sides l,wl,wA=lwA=lwP=2l+2wP=2l+2w
Circle, radius rrA=πr2A=\pi r^{2}C=2πrC=2\pi r
Right-angled triangle, perpendicular sides a,ba,b, hypotenuse ccA=12abA=\tfrac12abP=a+b+cP=a+b+c, with c=a2+b2c=\sqrt{a^{2}+b^{2}}
Isosceles triangle, base bb, height hh, equal sides ssA=12bhA=\tfrac12bhP=b+2sP=b+2s, with h=s2−(b/2)2h=\sqrt{s^{2}-(b/2)^{2}}

A triangular cross-section of area AA extended uniformly through length LL has volume ALAL, just as a cylinder has its circular cross-section multiplied by length.

SolidVolumeTotal surface area
Cuboid, sides l,w,hl,w,hV=lwhV=lwhS=2(lw+lh+wh)S=2(lw+lh+wh)
Closed cylinder, radius rr, length LLV=πr2LV=\pi r^{2}LS=2πrL+2πr2S=2\pi rL+2\pi r^{2}
Sphere, radius rrV=43πr3V=\tfrac43\pi r^{3}S=4πr2S=4\pi r^{2}

These geometry relations are not on the data sheet: learn them. The cylinder's total surface area includes both circular ends; an open tube needs the appropriate surfaces instead. A hollow shape's material volume is the outer volume minus the empty inner volume.

Worked example 1: density of a rectangular sample

Question. A solid sample has mass 1.35 kg1.35\,\mathrm{kg} and dimensions 10.0 cm10.0\,\mathrm{cm}, 5.00 cm5.00\,\mathrm{cm} and 3.00 cm3.00\,\mathrm{cm}. Calculate its density.

V=0.100×0.0500×0.0300=1.50×10−4 m3ρ=1.351.50×10−4=9.00×103 kg m−3\begin{aligned} V&=0.100\times0.0500\times0.0300=1.50\times10^{-4}\,\mathrm{m^{3}}\\ \rho&=\frac{1.35}{1.50\times10^{-4}}=9.00\times10^{3}\,\mathrm{kg\,m^{-3}} \end{aligned}

Answer. 9.00×103 kg m−39.00\times10^{3}\,\mathrm{kg\,m^{-3}}.

Check. The volume is 150 cm3150\,\mathrm{cm^{3}}, not 150 m3150\,\mathrm{m^{3}}. The mass of one cubic metre is much larger than that of this small sample.

A sphere illustrates why surface area and volume must not be confused: doubling its radius multiplies its surface area by four but its volume, and hence its mass at fixed density, by eight. This is a consequence of the powers of radius in the geometry, not a change in the material.

Exam-style example: density from a diameter

Question. A solid sphere of diameter 0.0300 m0.0300\,\mathrm{m} has mass 0.0380 kg0.0380\,\mathrm{kg}. Calculate its density.

Plan. Halve the diameter, calculate the sphere's volume, then use mass per unit volume.

r=0.0150 mV=43π(0.0150)3=1.414×10−5 m3ρ=0.03801.414×10−5=2.69×103 kg m−3\begin{aligned} r&=0.0150\,\mathrm{m}\\ V&=\tfrac43\pi(0.0150)^3=1.414\times10^{-5}\,\mathrm{m^{3}}\\ \rho&=\frac{0.0380}{1.414\times10^{-5}}=2.69\times10^{3}\,\mathrm{kg\,m^{-3}} \end{aligned}

Check. Using diameter as radius would make the volume eight times too large and the density eight times too small.

For an irregular solid that does not dissolve or absorb water, immerse it fully and measure the increase in water volume in a measuring cylinder. Avoid trapped bubbles. Determine its mass separately with a balance. A small volume change has a large fractional uncertainty, so a suitably sized cylinder helps more than writing extra decimal places.

Normal force per unit area

The same force can have a very different effect when concentrated onto a small area. That is why a sharp point can penetrate a surface with a modest force, while spreading the force across a broad contact area reduces the pressure.

Pressure

Pressure is the normal force acting per unit area.

“Normal” means perpendicular to the surface. For a force perpendicular to a flat surface, pressure compares that force with the area over which it acts.

Pressure

p=FAp=\frac{F}{A}

Here pp is pressure in pascals, Pa\mathrm{Pa}, FF is the normal force in N\mathrm{N}, and AA is the area in m2\mathrm{m^{2}}. One pascal is one newton per square metre. For varying pressure this relation gives the average pressure over the stated area.

Not on the data sheet: learn it.

A fluid at rest exerts pressure normal to any surface in contact with it. Pressure at a point is a scalar; the associated force has a direction set by the surface. Fluid pressure is not a downward force simply because the fluid has weight.

Worked example 2: spreading a load

Question. A normal force of 250 N250\,\mathrm{N} acts uniformly over an area of 0.020 m20.020\,\mathrm{m^{2}}. Calculate the pressure.

p=2500.020=1.25×104 Pap=\frac{250}{0.020}=1.25\times10^{4}\,\mathrm{Pa}

Answer. About 1.3×104 Pa1.3\times10^{4}\,\mathrm{Pa}.

Check. Doubling the contact area with the same force would halve this pressure.

An area in square centimetres needs a squared conversion: 1 cm2=10−4 m21\,\mathrm{cm^{2}}=10^{-4}\,\mathrm{m^{2}}. Confusing a length conversion with an area conversion is a common source of powers-of-ten errors here.

Exam-style example: force on a circular piston

Question. Fluid exerts a uniform pressure of 9.5×104 Pa9.5\times10^{4}\,\mathrm{Pa} on one circular face of diameter 0.040 m0.040\,\mathrm{m}. Calculate the force on that face.

A=π(0.020)2=1.257×10−3 m2F=pA=(9.5×104)(1.257×10−3)=119 N\begin{aligned} A&=\pi(0.020)^2=1.257\times10^{-3}\,\mathrm{m^{2}}\\ F&=pA=(9.5\times10^{4})(1.257\times10^{-3})=119\,\mathrm{N} \end{aligned}

Answer. 1.2×102 N1.2\times10^{2}\,\mathrm{N}.

Check. This is the force from the fluid on that face, rather than necessarily the resultant on the whole piston. Pressure on its other face may exert an opposing force.

Use the actual loaded area, rather than the surface area of the whole object.

Pressure increases with vertical depth

A horizontal layer of fluid at rest must support the weight of the fluid above it. That creates a pressure increase with depth. Compare two levels within a fluid of uniform density, separated by a vertical distance Δh\Delta h.

Imagine a vertical cylinder of this fluid with cross-sectional area AA. Let its top and bottom pressures be p1p_1 and p2p_2. The fluid around it exerts an upward force p2Ap_2A on its bottom and a downward force p1Ap_1A on its top. Its weight is mgmg, so equilibrium gives

p2A−p1A=mgm=ρV=ρAΔh(p2−p1)A=ρAΔh gΔp=ρgΔh\begin{aligned} p_2A-p_1A&=mg\\ m&=\rho V=\rho A\Delta h\\ (p_2-p_1)A&=\rho A\Delta h\,g\\ \Delta p&=\rho g\Delta h \end{aligned}

The area cancels. This is why a narrow water tube and a wide water tank can have the same pressure at equal depth, even though their total water weights are very different.

[DIAGRAM: asset_name: Pressure difference in a stationary fluid; asset_slug: hydrostatic-cylinder; caption: The pressure force from below supports both the force from above and the cylinder's weight; description: A vertical imaginary cylinder inside a body of liquid has area A and height delta h. Downward top force p1 A and weight rho A delta h g act on it, while a larger upward bottom force p2 A balances their sum. Top and bottom levels are labelled p1 and p2.]
The pressure force from below supports both the force from above and the cylinder's weight

Hydrostatic pressure difference

Δp=ρgΔh\Delta p=\rho g\Delta h

Here Δp\Delta p is the pressure increase in Pa\mathrm{Pa} on going down through vertical depth Δh\Delta h in m\mathrm{m}, ρ\rho is the fluid density in kg m−3\mathrm{kg\,m^{-3}}, and gg is gravitational field strength in N kg−1\mathrm{N\,kg^{-1}}. The fluid is at rest, with approximately uniform density and gg. The simple form needs modification if density changes appreciably over the depth.

On the data sheet.

Pressure at a point below an open liquid surface is the pressure at the surface plus the extra hydrostatic pressure. With surface pressure p0p_0, the total is p=p0+ρghp=p_0+\rho gh, where hh is the vertical depth. This is the supplied pressure-difference relation applied between the surface and the point.

Worked example 3: extra pressure and total pressure

Question. A point is 0.85 m0.85\,\mathrm{m} below a water surface. The density is 1000 kg m−31000\,\mathrm{kg\,m^{-3}}, g=9.81 m s−2g=9.81\,\mathrm{m\,s^{-2}}, and surface pressure is 1.01×105 Pa1.01\times10^{5}\,\mathrm{Pa}. Calculate the extra pressure due to the water and the total pressure.

Δp=1000×9.81×0.85=8.34×103 Pap=1.01×105+8.34×103=1.09×105 Pa\begin{aligned} \Delta p&=1000\times9.81\times0.85=8.34\times10^{3}\,\mathrm{Pa}\\ p&=1.01\times10^{5}+8.34\times10^{3}\\ &=1.09\times10^{5}\,\mathrm{Pa} \end{aligned}

Check. The extra pressure is only about 8 kPa8\,\mathrm{kPa}; it is not the whole atmospheric-plus-water pressure.

A pressure-depth graph for a uniform liquid is a straight line with gradient ρg\rho g. If its vertical axis shows total pressure, its intercept at the surface is p0p_0; if it shows extra pressure above the surface value, its intercept is zero. For example, a pressure increase of 3.2×104 Pa3.2\times10^{4}\,\mathrm{Pa} through 4.0 m4.0\,\mathrm{m} gives ρ=Δp/(gΔh)=8.2×102 kg m−3\rho=\Delta p/(g\Delta h)=8.2\times10^{2}\,\mathrm{kg\,m^{-3}}. The slope, rather than the total pressure at one point, identifies density.

Watch out

Use the fluid's density and the vertical depth difference. The length of a sloping tube, the container's width and the density of an immersed object are not substitutes for those quantities.

Test the pressure difference without adding an unnecessary surface pressure.

Quick Recap

  • Density is mass per unit volume; use the correct geometric volume and convert lengths before taking powers.
  • Pressure is normal force per unit area, with one pascal equal to one newton per square metre.
  • A stationary uniform fluid has pressure difference equal to density times gravitational field strength times vertical depth difference.
  • Add the surface pressure when total pressure is required; pressure differences do not need that addition.

A narrow tube and a wide tank of the same stationary liquid have equal pressure at the same depth below surfaces at the same pressure: container width cancels from the force balance.