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Exercises · 9.19

Q.What is the pressure inside the drop of mercury of radius 3.00 mm3.00\ \text{mm} at room temperature? Surface tension of mercury at that temperature (20 ∘C20\,^{\circ}\text{C}) is 4.65×10−1 N m−14.65 \times 10^{-1}\ \text{N m}^{-1}. The atmospheric pressure is 1.01×105 Pa1.01 \times 10^{5}\ \text{Pa}. Also give the excess pressure inside the drop.

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The excess pressure inside a spherical liquid drop is given by ΔP=2Tr\Delta P = \frac{2T}{r}, where TT is surface tension and rr is radius. For a mercury drop of radius 3.00 mm3.00\ \text{mm} with T=4.65×10−1 N/mT = 4.65 \times 10^{-1}\ \text{N/m}, the excess pressure is 310 Pa310\ \text{Pa}. The total pressure inside is the sum of atmospheric pressure and this excess: 1.0131×105 Pa1.0131 \times 10^{5}\ \text{Pa}.

Why This Works — The Physics of Capillary Action

A liquid drop is not just a blob of fluid — it's held together by surface tension. The molecules at the surface experience a net inward pull because they have fewer neighbours on the outside. This creates a curved interface that is always under tension, like a stretched rubber membrane.

For a spherical drop, this tension tries to shrink the surface area. To keep the drop from collapsing, the pressure inside must be greater than the pressure outside. That difference — the excess pressure — is what we calculate.

The key formula comes from balancing forces on a hemisphere of the drop: the surface tension force around the circumference (T×2πrT \times 2\pi r) must equal the net pressure force on the flat circular face (ΔP×πr2\Delta P \times \pi r^2). Solving gives:

ΔP=2Tr\Delta P = \frac{2T}{r}

This is the Laplace pressure for a spherical interface with one free surface (a liquid drop in air). Notice: smaller radius → larger excess pressure. That's why tiny droplets are much harder to deform than large ones.


Step-by-Step Calculation

1. Identify the given data

  • Radius of mercury drop: r=3.00 mm=3.00×10−3 mr = 3.00\ \text{mm} = 3.00 \times 10^{-3}\ \text{m}
  • Surface tension of mercury at 20 ∘C20\,^{\circ}\text{C}: T=4.65×10−1 N/mT = 4.65 \times 10^{-1}\ \text{N/m}
  • Atmospheric pressure: Patm=1.01×105 PaP_{\text{atm}} = 1.01 \times 10^{5}\ \text{Pa}

2. Compute the excess pressure

Using ΔP=2Tr\Delta P = \frac{2T}{r}:

ΔP=2×4.65×10−13.00×10−3\Delta P = \frac{2 \times 4.65 \times 10^{-1}}{3.00 \times 10^{-3}}

First, multiply numerator: 2×4.65×10−1=9.30×10−1=0.9302 \times 4.65 \times 10^{-1} = 9.30 \times 10^{-1} = 0.930

Then divide: 0.9303.00×10−3=0.9300.00300=310 Pa\frac{0.930}{3.00 \times 10^{-3}} = \frac{0.930}{0.00300} = 310\ \text{Pa}

So the excess pressure is 310 Pa310\ \text{Pa}. …

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