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Exercises · 1.21

Q.A uniformly charged conducting sphere of 2.4 m2.4\,\text{m} diameter has a surface charge density of 80.0 μC/m280.0\,\mu\text{C/m}^2.

(a) Find the charge on the sphere.
(b) What is the total electric flux leaving the surface of the sphere?
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The total charge on the sphere is found by multiplying its surface charge density by its surface area. The total electric flux leaving the sphere is then calculated using Gauss's Law, which relates the flux to the total enclosed charge.

The charge on the sphere is 1.45×10−3 C\boxed{1.45 \times 10^{-3}\,\text{C}} and the total electric flux leaving its surface is 1.64×108 N⋅m2/C\boxed{1.64 \times 10^8\,\text{N}\cdot\text{m}^2/\text{C}}.

When dealing with charged objects, two fundamental quantities are often sought: the total charge and the electric flux. For a uniformly charged sphere, these calculations become straightforward due to its high degree of symmetry.

Concept and Intuition

  1. Surface Charge Density (σ\sigma): This quantity tells us how much charge is packed onto each unit area of a surface. If a charge QQ is spread uniformly over a surface area AA, then the surface charge density is simply Q/AQ/A. Conversely, if we know σ\sigma and AA, we can find the total charge Q=σAQ = \sigma A. For a sphere, the surface area is 4πR24\pi R^2.

  2. Gauss's Law: This is one of Maxwell's equations and a cornerstone of electrostatics. It provides a powerful way to calculate electric flux, especially for symmetric charge distributions. Gauss's Law states that the total electric flux (ΦE\Phi_E) through any closed surface (called a Gaussian surface) is directly proportional to the total electric charge (QencQ_{enc}) enclosed within that surface.

    ΦE=∮E⃗⋅dA⃗=Qencϵ0\Phi_E = \oint \vec{E} \cdot d\vec{A} = \frac{Q_{enc}}{\epsilon_0}

    Here, ϵ0\epsilon_0 is the permittivity of free space, a fundamental constant.

    For a uniformly charged sphere, the electric field lines point radially outward (if positive charge) or inward (if negative charge). If we choose a spherical Gaussian surface concentric with the charged sphere, the electric field E⃗\vec{E} will be uniform in magnitude and perpendicular to the surface everywhere. This simplifies the flux integral significantly, making Gauss's Law the ideal tool for this problem.


Let's solve the problem step-by-step.

Given Data:

  • Diameter of the sphere, D=2.4 mD = 2.4\,\text{m}
  • Surface charge density, σ=80.0 μC/m2\sigma = 80.0\,\mu\text{C/m}^2

We need to convert the surface charge density to standard SI units:

σ=80.0×10−6 C/m2\sigma = 80.0 \times 10^{-6}\,\text{C/m}^2


(a) Find the charge on the sphere.

  1. Calculate the radius of the sphere:

    The radius RR is half of the diameter.

    R=D2=2.4 m2=1.2 mR = \frac{D}{2} = \frac{2.4\,\text{m}}{2} = 1.2\,\text{m}

  2. Calculate the surface area of the sphere:

    The surface area AA of a sphere is given by the formula A=4πR2A = 4\pi R^2.

    A=4π(1.2 m)2A = 4\pi (1.2\,\text{m})^2

    A=4π(1.44 m2)A = 4\pi (1.44\,\text{m}^2)

    A=5.76π m2A = 5.76\pi\,\text{m}^2

  3. Calculate the total charge on the sphere:

    The total charge QQ is the product of the surface charge density σ\sigma and the surface area AA.

    Q=σAQ = \sigma A

    Q=(80.0×10−6 C/m2)×(5.76π m2)Q = (80.0 \times 10^{-6}\,\text{C/m}^2) \times (5.76\pi\,\text{m}^2)

    Q=460.8π×10−6 CQ = 460.8\pi \times 10^{-6}\,\text{C}

    Now, substitute the numerical value of π≈3.14159\pi \approx 3.14159:

    Q≈460.8×3.14159×10−6 CQ \approx 460.8 \times 3.14159 \times 10^{-6}\,\text{C}

    Q≈1447.645×10−6 CQ \approx 1447.645 \times 10^{-6}\,\text{C}

    Q≈1.447645×10−3 CQ \approx 1.447645 \times 10^{-3}\,\text{C}

    Rounding to three significant figures (consistent with 80.0 μC/m280.0\,\mu\text{C/m}^2):

    Q≈1.45×10−3 CQ \approx 1.45 \times 10^{-3}\,\text{C}

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