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Physics · Ch 9 — Mechanical Properties of Fluids

Atmospheric Pressure and Gauge Pressure

9.2.3

Atmospheric Pressure and Gauge Pressure

The Idea of Pressure

A sharp needle pressed into the skin pierces it easily, while a blunt spoon pressed with the same force does not. An elephant stepping on a man’s chest would crack his ribs, yet a circus performer can lie on a bed of nails without injury. The difference in each case is not the force applied, but how that force is distributed over the area of contact.

When force is concentrated over a tiny area, the effect is intense. When the same force is spread over a large area, the effect is mild. This leads to the definition of pressure — the normal force per unit area.

P=F⊥AP = \frac{F_{\perp}}{A}

Here F⊥F_{\perp} is the component of force acting perpendicular (normal) to the surface, and AA is the area over which the force is distributed. Pressure is a scalar quantity — it has magnitude but no direction. The SI unit of pressure is the pascal (Pa), where 1 Pa=1 N m−21 \text{ Pa} = 1 \text{ N m}^{-2}.

Watch out

A common mistake is to think pressure is a vector because force is a vector. Pressure is defined as the magnitude of the normal force per unit area — it has no direction associated with it. The force on a surface element is F⃗=P ΔA n^\vec{F} = P \, \Delta A \, \hat{n}, where n^\hat{n} is the unit normal to the surface; the pressure itself is just the scalar PP.

Atmospheric Pressure

The atmosphere surrounding the Earth exerts pressure on every surface in contact with it. This is called atmospheric pressure, denoted by PatmP_{\text{atm}}. At sea level, the standard value is:

Patm=1.013×105 PaP_{\text{atm}} = 1.013 \times 10^{5} \text{ Pa}

This is also known as 1 atmosphere (1 atm). In other common units:

1 atm=1.013×105 Pa=1.013 bar=760 mm of Hg1 \text{ atm} = 1.013 \times 10^{5} \text{ Pa} = 1.013 \text{ bar} = 760 \text{ mm of Hg}

The value 760 mm of Hg760 \text{ mm of Hg} comes from the classic experiment by Torricelli, where a column of mercury in a tube, inverted in a dish of mercury, stands at a height of about 76 cm at sea level. The pressure exerted by this mercury column exactly balances the atmospheric pressure pushing up on the mercury in the dish.

Note

The exact value of atmospheric pressure varies with altitude, weather conditions, and temperature. The standard value 1.013×105 Pa1.013 \times 10^{5} \text{ Pa} is a reference point, not a constant everywhere on Earth.

Properties of Fluid Pressure

The textbook lists several key properties of pressure in a fluid at rest. Each one is derived from the fundamental definition and the condition of equilibrium.

›Proof

Property 1: Pressure is the same in all directions in a fluid at rest.

Consider a tiny, wedge-shaped element of fluid at rest, with dimensions Δx\Delta x, Δy\Delta y, and Δz\Delta z (the wedge has a sloping face of length Δs\Delta s). The wedge is so small that the pressure can be taken as uniform over each face. Let PxP_x, PyP_y, and PsP_s be the pressures on the faces perpendicular to the xx-axis, yy-axis, and the sloping face respectively. The forces on the wedge are:

  • On the face perpendicular to xx: Fx=Px (Δy⋅Δz)F_x = P_x \, (\Delta y \cdot \Delta z) (acting in the +x+x direction)
  • On the face perpendicular to yy: Fy=Py (Δx⋅Δz)F_y = P_y \, (\Delta x \cdot \Delta z) (acting in the +y+y direction)
  • On the sloping face: Fs=Ps (Δs⋅Δz)F_s = P_s \, (\Delta s \cdot \Delta z) (acting normal to the sloping face)
  • The weight of the fluid element: W=ρg (volume)=ρg(12ΔxΔyΔz)W = \rho g \, (\text{volume}) = \rho g \left( \frac{1}{2} \Delta x \Delta y \Delta z \right) (acting vertically downward)

For equilibrium, the net force in the xx-direction must be zero. The xx-component of FsF_s is Fssin⁡θ=Ps(Δs⋅Δz)sin⁡θF_s \sin \theta = P_s (\Delta s \cdot \Delta z) \sin \theta. From the geometry of the wedge, Δy=Δssin⁡θ\Delta y = \Delta s \sin \theta. So the xx-component of FsF_s is Ps(Δy⋅Δz)P_s (\Delta y \cdot \Delta z). The force FxF_x acts in the −x-x direction (it pushes the wedge to the left). Therefore:

Px(Δy⋅Δz)−Ps(Δy⋅Δz)=0P_x (\Delta y \cdot \Delta z) - P_s (\Delta y \cdot \Delta z) = 0

This gives Px=PsP_x = P_s.

Similarly, for equilibrium in the yy-direction, the yy-component of FsF_s is Fscos⁡θ=Ps(Δs⋅Δz)cos⁡θF_s \cos \theta = P_s (\Delta s \cdot \Delta z) \cos \theta. From geometry, Δx=Δscos⁡θ\Delta x = \Delta s \cos \theta, so this component is Ps(Δx⋅Δz)P_s (\Delta x \cdot \Delta z). The force FyF_y acts in the −y-y direction. The weight WW also has a component in the yy-direction? No — weight acts vertically, and in our coordinate system, yy is horizontal. So the yy-direction equilibrium is:

Py(Δx⋅Δz)−Ps(Δx⋅Δz)=0P_y (\Delta x \cdot \Delta z) - P_s (\Delta x \cdot \Delta z) = 0

This gives Py=PsP_y = P_s.

Since Px=PsP_x = P_s and Py=PsP_y = P_s, we have Px=Py=PsP_x = P_y = P_s. The choice of orientation of the wedge was arbitrary, so the pressure at a point in a static fluid is the same in all directions.

›Proof

Property 2: In a fluid at rest, the pressure is the same at all points on the same horizontal level.

Consider two points A and B at the same height in a static fluid. Imagine a small cylindrical element of fluid connecting them, with its axis horizontal. The only horizontal forces on this cylinder are the pressure forces on its two end faces. For the cylinder to be in equilibrium (no horizontal acceleration), these forces must be equal and opposite. Therefore, the pressure at A must equal the pressure at B. This holds for any two points at the same depth in a continuous, static fluid.

›Proof

Property 3: Pressure varies with depth in a fluid.

Consider a cylindrical column of fluid of height hh and cross-sectional area AA, extending from the free surface (where pressure is P0P_0, usually atmospheric pressure) down to a depth hh. The forces acting on this column are: …

Figure 9.5Two pressure measuring devices. (a) The mercury barometer. (b) The open tube manometer.
Fig. 9.5 — Two pressure measuring devices. (a) The mercury barometer. (b) The open tube manometer.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your textbook's own diagram.

Figure 9.5 places two classic pressure-measuring instruments side by side: the mercury barometer and the open-tube manometer. Both rely on the same core idea — a column of liquid balances an unknown pressure — but they answer different questions. The barometer measures atmospheric pressure; the manometer measures the pressure of a gas in a container relative to the atmosphere.

Panel (a) — The mercury barometer. A long glass tube, sealed at one end, is filled completely with mercury and then inverted into a trough of mercury. The mercury column drops until the pressure at the top of the column (point A) is essentially zero — a near-vacuum. At the bottom of the column, point B is at the mouth of the tube, level with the free surface of the mercury in the trough (point C). The free surface C is open to the atmosphere, so the pressure there is PatmP_{\text{atm}}. The column height hh is the vertical distance from the trough surface to the top of the mercury inside the tube.

The physics is a simple hydrostatic balance. The pressure at point B (inside the tube, at the same horizontal level as C) must equal the pressure at C, because in a static fluid the pressure is the same at all points on the same horizontal level. At B, the pressure is due only to the weight of the mercury column above it — the vacuum at A contributes nothing. Therefore:

Patm=ρHg g hP_{\text{atm}} = \rho_{\text{Hg}} \, g \, h

where ρHg\rho_{\text{Hg}} is the density of mercury, gg is the acceleration due to gravity, and hh is the column height. At sea level, h≈76 cmh \approx 76\ \text{cm} of mercury. This is the standard barometer equation: atmospheric pressure is directly proportional to the height of the mercury column it supports.

Watch out

The pressure at the top (point A) is not exactly zero — it is the vapour pressure of mercury, which is tiny at room temperature (about 0.0012 mm Hg0.0012\ \text{mm Hg}). For all practical purposes in Class 11, treat it as zero.

Panel (b) — The open-tube manometer. A U-shaped tube contains mercury. One arm (left) is connected to a bulb or container whose pressure PP we want to measure. The other arm (right) is open to the atmosphere, so the pressure at the free surface on that side is PatmP_{\text{atm}}. The mercury levels differ by a height hh: the column is higher on the side with lower pressure.

Again, use the principle that pressure is the same at all points on the same horizontal level in a connected static fluid. Choose the horizontal level that passes through the lower mercury surface in the open arm (point B). On the open side, the pressure at B is just PatmP_{\text{atm}}. On the left side, at the same level, the pressure is PP (the gas pressure in the bulb) plus the pressure due to the extra height hh of mercury above that level:

P+ρHg g h=PatmP + \rho_{\text{Hg}} \, g \, h = P_{\text{atm}}

The sign of hh matters. If the gas pressure is greater than atmospheric, the mercury is pushed down on the left and up on the right — then hh is positive and P=Patm+ρghP = P_{\text{atm}} + \rho g h. If the gas pressure is less than atmospheric, the mercury rises on the left and falls on the right — then hh is negative and P=Patm−ρg∣h∣P = P_{\text{atm}} - \rho g |h|. The manometer thus gives the gauge pressure (the difference from atmospheric) directly as ρgh\rho g h.

P=Patm±ρghP = P_{\text{atm}} \pm \rho g h …