A small bar magnet lies along the x-axis with its Centre fixed at the origin. If the magnetic field at point (5\(\hat{i}\)) m due to this magnet is 4x106 T,then the magnetic field at point (10\(\hat{j}\)) m will be :
2.5x 10-7 T
2x10-6 T
1x10-6 T
2.0x10-7 T
8.0x10-8 T
Given:
- The magnetic field at \((5 \hat{i})\) meters is \(4 \times 10^6 \, \text{T}\).
- We need to find the magnetic field at \((10 \hat{j})\) meters.
The magnetic field \(B\) due to a magnetic dipole at a distance \(r\) from the dipole along the axial (x-axis) direction is given by:
\[B_{\text{axial}} = \frac{\mu_0}{4\pi} \frac{2M}{r^3}\]
And along the equatorial (y-axis) direction is given by:
\[B_{\text{equatorial}} = \frac{\mu_0}{4\pi} \frac{M}{r^3}\]
where:
- \(M\) is the magnetic moment of the bar magnet,
- \(\mu_0\) is the permeability of free space (\(\mu_0 = 4\pi \times 10^{-7} \, \text{T} \cdot \text{m}/\text{A}\)).
Given the field along the x-axis (axial position) at \(r = 5 \, \text{m}\):
\[4 \times 10^6 \, \text{T} = \frac{\mu_0}{4\pi} \frac{2M}{(5)^3}\]
Simplifying:
\[4 \times 10^6 = \frac{2 \times 10^{-7} M}{125}\]
Solving for \(M\):
\[M = \frac{4 \times 10^6 \times 125}{2 \times 10^{-7}}\]
\[M = \frac{5 \times 10^8}{10^{-7}} = 2.5 \times 10^{15} \, \text{A} \cdot \text{m}^2\]
Now, we need to find the magnetic field at \((10 \hat{j})\) meters (equatorial position):
\[B_{\text{equatorial}} = \frac{\mu_0}{4\pi} \frac{M}{(10)^3}\]
\[B_{\text{equatorial}} = \frac{10^{-7} \times 2.5 \times 10^{15}}{1000}\]
\[B_{\text{equatorial}} = 2.5 \times 10^{-7} \, \text{T}\]
Therefore, the magnetic field at the point \((10 \hat{j})\) meters is \(2.5 \times 10^{-7} \, \text{T}\),
So The correct answer is Option(A): 2.5x 10-7 T
Step 1: Understand the magnetic field due to a bar magnet.
The magnetic field due to a bar magnet depends on:
For a bar magnet lying along the x-axis with its center at the origin:
\[ B_{\text{axial}} = \frac{\mu_0}{4\pi} \cdot \frac{2M}{r^3}, \]
\[ B_{\text{equatorial}} = \frac{\mu_0}{4\pi} \cdot \frac{M}{r^3}. \] Thus, the relationship between the axial and equatorial fields at the same distance \( r \) is: \[ B_{\text{equatorial}} = \frac{B_{\text{axial}}}{2}. \] However, in this problem, the distances along the axial and equatorial lines are different, so we must account for the dependence on \( r^3 \).
Step 2: Analyze the given data.
We are given:
Step 3: Relate the magnetic fields using the formula.
The magnetic field along the axial line is: \[ B_{\text{axial}} = \frac{\mu_0}{4\pi} \cdot \frac{2M}{r_{\text{axial}}^3}. \] The magnetic field along the equatorial line is: \[ B_{\text{equatorial}} = \frac{\mu_0}{4\pi} \cdot \frac{M}{r_{\text{equatorial}}^3}. \] Dividing these two equations, we get: \[ \frac{B_{\text{equatorial}}}{B_{\text{axial}}} = \frac{\frac{M}{r_{\text{equatorial}}^3}}{\frac{2M}{r_{\text{axial}}^3}} = \frac{r_{\text{axial}}^3}{2r_{\text{equatorial}}^3}. \] Substitute the given distances: \[ r_{\text{axial}} = 5 \, \text{m}, \quad r_{\text{equatorial}} = 10 \, \text{m}. \] Thus: \[ \frac{B_{\text{equatorial}}}{B_{\text{axial}}} = \frac{(5)^3}{2(10)^3} = \frac{125}{2(1000)} = \frac{125}{2000} = \frac{1}{16}. \] Now, solve for \( B_{\text{equatorial}} \): \[ B_{\text{equatorial}} = \frac{1}{16} \cdot B_{\text{axial}}. \] Substitute \( B_{\text{axial}} = 4 \times 10^{-6} \, \text{T} \): \[ B_{\text{equatorial}} = \frac{1}{16} \cdot 4 \times 10^{-6} = 0.25 \times 10^{-6} = 2.5 \times 10^{-7} \, \text{T}. \]
Final Answer: The magnetic field at point \( (10\hat{j}) \, \text{m} \) is \( \mathbf{2.5 \times 10^{-7} \, \text{T}} \), which corresponds to option \( \mathbf{(A)} \).
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
The magnetic field is a field created by moving electric charges. It is a force field that exerts a force on materials such as iron when they are placed in its vicinity. Magnetic fields do not require a medium to propagate; they can even propagate in a vacuum. Magnetic field also referred to as a vector field, describes the magnetic influence on moving electric charges, magnetic materials, and electric currents.