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Question: The illuminance of a surface distance 10 m from a light source is 10 lux. The luminous intensity of ...

The illuminance of a surface distance 10 m from a light source is 10 lux. The luminous intensity of the source for normal incidence will be
(A) 101Cd{10^1}Cd
(B) 102Cd{10^2}Cd
(C) 103Cd{10^3}Cd
(D) None of these

Explanation

Solution

Illuminance is defined as the luminous flux per unit surface area. While luminous flux is the luminous intensity through a unit solid angle. Assume the source light diverges in all directions.

Formula used: In this solution we will be using the following formulae:
Ev=ϕv4πR2\Rightarrow {E_v} = \dfrac{{{\phi _v}}}{{4\pi {R^2}}} , where Ev{E_v} is the illuminance, ϕv{\phi _v} is the luminous flux, and RR is the distance of the surface from the source.
lv=ϕvθ\Rightarrow {l_v} = \dfrac{{{\phi _v}}}{\theta } where lv{l_v} is the luminous intensity and θ\theta is the solid angle measured in Steradians.

Complete step by step solution:
The illuminance of a surface is the luminous flux incident on that surface. It is given as luminous flux per unit area.
For a source, diverging in all directions, we have that the total surface area is the surface area of a sphere, hence A=4πR2A = 4\pi {R^2} . Then the illuminance becomes
Ev=ϕv4πR2\Rightarrow {E_v} = \dfrac{{{\phi _v}}}{{4\pi {R^2}}}
Calculating luminous flux by inserting all known values, we have
ϕv=Ev×4πR2=10×4π(102)=4π×103lm\Rightarrow {\phi _v} = {E_v} \times 4\pi {R^2} = 10 \times 4\pi \left( {{{10}^2}} \right) = 4\pi \times {10^3}lm , lmlm is called the lumen.
Now, luminous intensity is given by the luminous flux per unit solid angle. Hence
lv=ϕvθ\Rightarrow {l_v} = \dfrac{{{\phi _v}}}{\theta } where lv{l_v} is the luminous intensity and θ\theta is the solid angle measured in Steradians.
For a complete sphere, the solid angle subtended is 4π4\pi i.e. θ=4π\theta = 4\pi (analogous to a circle subtending a plane angle of 2π2\pi ).
Hence,
lv=ϕvθ=4π×1034π=103cd\Rightarrow {l_v} = \dfrac{{{\phi _v}}}{\theta } = \dfrac{{4\pi \times {{10}^3}}}{{4\pi }} = {10^3}cd
Hence the correct option is C.

Note:
Alternatively, without firstly calculating the flux, we substitute the expression for luminous flux as a function of luminous intensity into Ev=ϕv4πR2{E_v} = \dfrac{{{\phi _v}}}{{4\pi {R^2}}} as in:
From
lv=ϕvθϕv=lvθ\Rightarrow {l_v} = \dfrac{{{\phi _v}}}{\theta } \Rightarrow {\phi _v} = {l_v}\theta
Hence, Ev=ϕv4πR2{E_v} = \dfrac{{{\phi _v}}}{{4\pi {R^2}}} becomes
Ev=lvθ4πR2\Rightarrow {E_v} = \dfrac{{{l_v}\theta }}{{4\pi {R^2}}} . Making lv{l_v} subject we have
lv=Ev×4πR2θ\Rightarrow {l_v} = \dfrac{{{E_v} \times 4\pi {R^2}}}{\theta }
Inserting values, we get
lv=10×4π×1024π=103cd\Rightarrow {l_v} = \dfrac{{10 \times 4\pi \times {{10}^2}}}{{4\pi }} = {10^3}cd