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Physics · Ch 9 — Mechanical Properties of Fluids

Capillary Rise

9.6.5

Capillary Rise

Capillary Rise

When a narrow tube (a capillary) is dipped into a liquid, the liquid either rises or falls inside the tube relative to the surrounding liquid surface. This phenomenon is called capillarity or capillary action. The rise of a liquid in a capillary tube is one of the most direct demonstrations of surface tension at work.

The key observation is this: if the liquid wets the tube (like water in glass), it rises up the tube. If the liquid does not wet the tube (like mercury in glass), it is depressed below the surrounding level. The height of rise or depression depends on the tube's radius, the liquid's surface tension, and the contact angle between the liquid and the tube material.

The Mechanism Behind Capillary Rise

Consider a glass capillary tube dipped vertically into water. Water molecules are strongly attracted to the glass — the adhesive force between water and glass is greater than the cohesive force between water molecules. This causes the water surface at the contact line to curve upward, forming a concave meniscus.

The curved meniscus creates a pressure difference across the liquid-air interface. According to the Young-Laplace equation, the pressure just below a concave meniscus is less than the atmospheric pressure above it. This lower pressure pulls the liquid up the tube until the hydrostatic pressure of the raised column balances the pressure deficit.

Note

The same principle explains why a liquid rises in a blotting paper or a wick — the fibres act as many narrow capillaries.

Deriving the Height of Capillary Rise

Let a capillary tube of radius rr be dipped vertically into a liquid of density ρ\rho and surface tension SS. The liquid makes a contact angle θ\theta with the tube wall. The meniscus is approximately spherical, with radius of curvature RR.

From the geometry of the meniscus, the radius of curvature RR is related to the tube radius rr and the contact angle θ\theta by:

R=rcos⁡θR = \frac{r}{\cos \theta}

The pressure difference across the curved liquid-air interface is given by the Young-Laplace equation for a spherical surface:

ΔP=2SR\Delta P = \frac{2S}{R}

Substituting R=r/cos⁡θR = r/\cos \theta:

ΔP=2Scos⁡θr\Delta P = \frac{2S \cos \theta}{r}

This pressure difference is the driving force. The pressure just below the meniscus is Patm−ΔPP_{\text{atm}} - \Delta P, while the pressure at the same horizontal level outside the tube is PatmP_{\text{atm}}. The liquid rises to a height hh such that the hydrostatic pressure of the column of height hh exactly balances this pressure difference:

ρgh=ΔP=2Scos⁡θr\rho g h = \Delta P = \frac{2S \cos \theta}{r}

Therefore, the height of capillary rise is:

h=2Scos⁡θρgrh = \frac{2S \cos \theta}{\rho g r}

h=2Scos⁡θρgrh = \frac{2S \cos \theta}{\rho g r}

This is the central result for capillary rise.

Important Consequences and Properties

Property 1: Height is inversely proportional to tube radius.

From the formula, h∝1/rh \propto 1/r. A narrower tube produces a greater rise. This is why water rises higher in a thin capillary than in a wider one. For a given liquid and tube material, halving the radius doubles the rise height.

Property 2: The rise depends on the contact angle.

For a wetting liquid (θ<90∘\theta < 90^\circ), cos⁡θ\cos \theta is positive, so hh is positive — the liquid rises. For a non-wetting liquid (θ>90∘\theta > 90^\circ), cos⁡θ\cos \theta is negative, so hh is negative — the liquid is depressed below the surrounding level. For θ=0∘\theta = 0^\circ (perfect wetting), cos⁡θ=1\cos \theta = 1 and the rise is maximum for that radius:

hmax=2Sρgrh_{\text{max}} = \frac{2S}{\rho g r}

For θ=90∘\theta = 90^\circ, cos⁡θ=0\cos \theta = 0 and there is no rise or depression — the liquid surface remains flat.

Watch out

A common mistake is to forget that θ\theta can be greater than 90∘90^\circ. For mercury in glass, θ≈140∘\theta \approx 140^\circ, so cos⁡θ\cos \theta is negative, giving a negative hh — the mercury is depressed, not raised.

Property 3: The meniscus is approximately spherical.

For a narrow tube, the meniscus is very nearly a spherical surface. The radius of curvature RR is constant over the entire meniscus. This approximation breaks down for very wide tubes, where the meniscus becomes flatter near the centre.

Property 4: The rise height is independent of the tube's length (as long as it is long enough).

If the tube is shorter than the calculated rise height, the liquid will rise to the top and form a curved surface at the rim — the formula no longer applies. The liquid will not overflow; instead, the meniscus adjusts its curvature until the pressure balance is satisfied at the top.

The Complete Derivation (Step by Step)

›Proof

Full derivation of capillary rise height

Step 1: Geometry of the meniscus

The meniscus is a spherical cap of radius RR. The tube radius rr and the contact angle θ\theta are related by the right triangle formed by the tube wall, the tangent to the meniscus at the contact line, and the radius of curvature:

cos⁡θ=rR\cos \theta = \frac{r}{R}

Hence R=r/cos⁡θR = r / \cos \theta.

Step 2: Pressure difference across the curved surface

For a spherical liquid-air interface, the Young-Laplace equation gives:

Pinside−Poutside=−2SRP_{\text{inside}} - P_{\text{outside}} = -\frac{2S}{R}

The sign convention: for a concave meniscus (wetting liquid), the centre of curvature lies outside the liquid, so the pressure inside the liquid is less than outside. Taking PatmP_{\text{atm}} as the outside pressure:

Pliquid=Patm−2SRP_{\text{liquid}} = P_{\text{atm}} - \frac{2S}{R}

The pressure deficit is ΔP=2S/R\Delta P = 2S/R.

Step 3: Hydrostatic balance

At the same horizontal level as the free surface outside the tube, the pressure in the liquid outside is PatmP_{\text{atm}}. Inside the tube, at that same level, the pressure is Pliquid+ρghP_{\text{liquid}} + \rho g h (since we go down a distance hh from the meniscus). For equilibrium:

Patm=Pliquid+ρghP_{\text{atm}} = P_{\text{liquid}} + \rho g h

Substituting PliquidP_{\text{liquid}}:

Patm=(Patm−2SR)+ρghP_{\text{atm}} = \left(P_{\text{atm}} - \frac{2S}{R}\right) + \rho g h

ρgh=2SR\rho g h = \frac{2S}{R}

Step 4: Substitute for RR

ρgh=2Scos⁡θr\rho g h = \frac{2S \cos \theta}{r}

h=2Scos⁡θρgrh = \frac{2S \cos \theta}{\rho g r}

This completes the derivation.

Numerical Example …

Figure 9.19Capillary rise, (a) Schematic picture of a narrow tube immersed water. (b) Enlarged picture near interface.
Fig. 9.19 — Capillary rise, (a) Schematic picture of a narrow tube immersed water. (b) Enlarged picture near interface.

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 9.19 is the textbook’s visual anchor for understanding capillary rise — the phenomenon where a liquid climbs up a narrow tube against gravity. The figure has two parts, (a) and (b), each showing a different scale of the same situation.

Part (a) is the wide view. A narrow glass tube stands vertically in a large vessel of water. The water surface outside the tube is flat and horizontal; a point on that outer surface is labelled A. Inside the tube, the water has risen to a height hh above the outer level. The top of the water column inside the tube is not flat — it is curved, forming a meniscus. The lowest point of that meniscus is labelled B. The pressure at the top of the tube (above the meniscus) is atmospheric pressure PaP_a. Just below the concave meniscus, the pressure is P0P_0, which is less than PaP_a because the curved surface pulls inward. This pressure difference is what supports the column of height hh.

Part (b) zooms in on the meniscus region. The tube has internal radius aa. The meniscus is concave upward (like a bowl), with radius of curvature rr. At the point where the meniscus meets the tube wall, the liquid surface makes an angle θ\theta with the wall — this is the contact angle. For water in clean glass, θ\theta is nearly zero, so the meniscus is almost hemispherical. The figure makes clear that the radius of curvature rr is related to the tube radius aa by a=rcos⁡θa = r \cos \theta.

Important

The entire physics of capillary rise hinges on the pressure difference across a curved liquid surface. For a concave meniscus, the pressure just below the surface is lower than the pressure just above it.

The textbook uses this figure to derive the key formula for the height hh of capillary rise. The pressure difference across the curved meniscus is given by the Young–Laplace equation:

Pa−P0=2SrP_a - P_0 = \frac{2S}{r}

where SS is the surface tension of the liquid. This pressure difference must balance the hydrostatic pressure of the column of height hh:

Pa−P0=ρghP_a - P_0 = \rho g h

where ρ\rho is the density of the liquid and gg is the acceleration due to gravity. Equating the two expressions and using r=a/cos⁡θr = a / \cos \theta gives the capillary rise formula:

h=2Scos⁡θρgah = \frac{2S \cos \theta}{\rho g a}

Here aa is the tube radius, θ\theta is the contact angle, SS is surface tension, ρ\rho is liquid density, and gg is gravity. The formula shows that hh is inversely proportional to the tube radius — narrower tubes give higher rise. For water in glass, cos⁡θ≈1\cos \theta \approx 1, so h≈2S/(ρga)h \approx 2S / (\rho g a). …