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Exercises · 5.7

Q.A short bar magnet has a magnetic moment of 0.48 J T−10.48\ \text{J T}^{-1}. Give the direction and magnitude of the magnetic field produced by the magnet at a distance of 10 cm10\ \text{cm} from the centre of the magnet on

(a) the axis,
(b) the equatorial lines (normal bisector) of the magnet.
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The magnetic field of a short bar magnet is derived from its magnetic moment using the axial and equatorial formulas. At 10 cm10\ \text{cm} from the centre, the axial field is 0.96×10−4 T0.96 \times 10^{-4}\ \text{T} directed away from the north pole, and the equatorial field is 0.48×10−4 T0.48 \times 10^{-4}\ \text{T} directed opposite to the magnetic moment.

The key to solving this lies in understanding that a bar magnet behaves like a magnetic dipole. Its magnetic moment M\mathbf{M} is a vector pointing from the south pole to the north pole inside the magnet. The field it produces at any point depends on the orientation of that point relative to the dipole axis.

For a short magnet (length much smaller than the distance rr), we use the dipole approximation. This is valid here because the distance 10 cm10\ \text{cm} is large compared to the magnet's length (which is not given but implied to be small). The formulas are exact for a point dipole and excellent approximations for a short bar magnet.

For a magnetic dipole of moment MM:

  • Axial field (on the axis, at distance rr from centre): Baxis=μ04π⋅2Mr3B_{\text{axis}} = \frac{\mu_0}{4\pi} \cdot \frac{2M}{r^3}
  • Equatorial field (on the perpendicular bisector, at distance rr): Beq=μ04π⋅Mr3B_{\text{eq}} = \frac{\mu_0}{4\pi} \cdot \frac{M}{r^3}

Notice the factor of 2 difference: the axial field is twice the equatorial field at the same distance. This is a direct consequence of the dipole field geometry — field lines are denser along the axis.

Now let's apply these to the given data.

  1. Write down the known quantities.

    Magnetic moment M=0.48 J T−1M = 0.48\ \text{J T}^{-1} (which is equivalent to A m2\text{A m}^2).

    Distance r=10 cm=0.10 mr = 10\ \text{cm} = 0.10\ \text{m}.

    The constant μ04π=10−7 T m A−1\frac{\mu_0}{4\pi} = 10^{-7}\ \text{T m A}^{-1} (exactly, by definition of the ampere).

  2. Calculate the axial field.

Baxis=10−7×2×0.48(0.10)3B_{\text{axis}} = 10^{-7} \times \frac{2 \times 0.48}{(0.10)^3}

First, (0.10)3=0.001=10−3(0.10)^3 = 0.001 = 10^{-3}.

So Baxis=10−7×0.9610−3=10−7×0.96×103=0.96×10−4 TB_{\text{axis}} = 10^{-7} \times \frac{0.96}{10^{-3}} = 10^{-7} \times 0.96 \times 10^{3} = 0.96 \times 10^{-4}\ \text{T}.

That is 9.6×10−5 T9.6 \times 10^{-5}\ \text{T}.

Direction: On the axis, the field points away from the north pole and toward the south pole. Since the magnetic moment points from south to north, the axial field is parallel to M\mathbf{M} on the side of the north pole, and antiparallel on the south pole side. The problem asks for "direction" — we state it as along the axis, away from the north pole (or equivalently, in the direction of M\mathbf{M} if the point is on the north side).

  1. Calculate the equatorial field. …

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