Planck’s Radiation Law and Solar Constant
Plank's law for short distance is Wien's law and for long wavelength is Rayleigh jeans law. This note provides us an information on Planck’s radiation law and solar constant.
Summary
Plank's law for short distance is Wien's law and for long wavelength is Rayleigh jeans law. This note provides us an information on Planck’s radiation law and solar constant.
Things to Remember
- For shorter wave length \(\therefore E_{\lambda }d\lambda = \frac {8\pi hc\:e^{-\frac {h}{\lambda KT}}}{\lambda^5}d\lambda\) which is Wein's law.
- For longer wavelength,\( E_{\lambda }d\lambda = \frac {8\pi KT}{\lambda ^4}d\lambda \)
which is Rayleigh Jeans law.
- Wien’s Law holds for shorter wavelength while Rayleigh-Jeans law holds true for longer wavelength.
- The solar constant is defined as the amount of solar energy received per minute by unit area of a perfectly black body placed at a mean distance of the earth from the sun, in absence of the atmosphere and at right angle to the direction of sun’s rays.
MCQs
No MCQs found.
Subjective Questions
Q1:
Determine whether the following are terminating or repeating decimals.
\(\frac{2}{5}\)
Type: Short Difficulty: Easy
<p>\(\frac{2}{5}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.4\\[-3pt]5\enclose{longdiv} {20}\\[-3pt]\underline{20} \end{array}\) </p>
<p>Here, Divident = 2</p>
<p> Divisor = 5</p>
Q2:
Determine whether the following are terminating or repeating decimals.
\(\frac{1}{2}\)
Type: Short Difficulty: Easy
<p>\(\frac{1}{2}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.5\\[-3pt]2\enclose{longdiv} {10}\\[-3pt]\underline{10} \end{array}\) </p>
<p> Divident = 1</p>
<p> Divisor = 2</p>
<p>Here, \(\frac{1}{2}\)= 0.5 which is terminating decimal. </p>
<p> </p>
Q3:
Determine whether the following are terminating or repeating decimals.
\(\frac{11}{30}\)
Type: Long Difficulty: Easy
<p>= \(\frac{11}{30}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.366\\[-3pt]30\enclose{longdiv}{110}\\[-3pt]\underline{90}\\[-3pt]{200} \\[-3pt]\underline{180}\\[-3pt]\\{200}\\[-3pt]\underline{180}\\[-3pt]{20}\end{array}\)</p>
<p>Divident= 11</p>
<p>Divisor= 30</p>
<p>Here, \(\frac{11}{30}\) = 0.366 is also repeating decimal. So it is rational number. </p>
<p> </p>
Q4:
Determine whether the following are terminating or repeating decimals.
\(\frac{7}{22}\)
Type: Long Difficulty: Easy
<p>=\(\frac{7}{22}\)</p>
<p>= \(\require{enclose}\begin{array}{r}1.31818\\[-3pt]22\enclose{longdiv}{70}\\[-3pt]\underline{66}\\[-3pt]{40} \\[-3pt]\underline{22}\\[-3pt]\\{180}\\[-3pt]\underline{176}\\[-3pt]{40}\\[-3pt]\underline{22}\\[-3pt]{180}\\[-3pt]\underline{176}\\{4}\end{array}\)</p>
<p>Divident= 7</p>
<p>Divisor= 22</p>
<p>Here, \(\frac{7}{22}\) = 0.31818 which is repeating decimal. So, \(\frac{7}{22}\) is a rational number. </p>
Q5:
What are whole numbers?
Type: Very_short Difficulty: Easy
Q6:
What are a Rational number?
Type: Very_short Difficulty: Easy
Q7:
What does zero denote in Natural Number System?
Type: Very_short Difficulty: Easy
Q8:
What are positive Integers?
Type: Very_short Difficulty: Easy
Q9:
What are integers?
Type: Very_short Difficulty: Easy
Q10:
Determine whether the following are terminating or repeating decimals.
\(\frac{1}{4}\)
Type: Short Difficulty: Easy
<p>=\(\frac{1}{4}\)</p>
<p> </p>
<p>=\(\require{enclose}\begin{array}{r}0.25\\[-3pt]4\enclose{longdiv}{10}\\[-3pt]\underline{8}\\[-3pt]{20}\\\underline{20}\end{array}\)</p>
<p>Divident = 1</p>
<p>Divisor= 4</p>
<p>Here, \(\frac{1}{4}\) = 0.25 which is terminating decimal. </p>
Q11:
Determine whether the following are terminating or repeating decimals.
\(\frac{1}{4}\)
Type: Short Difficulty: Easy
<p>\(\frac{1}{4}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.25\\[-3pt]4\enclose{longdiv} {10}\\[-3pt]\underline{8} \\[-3pt]20\\\underline{20}\end{array}\) </p>
<p>= Here, the quotient is 0.25. It is terminating after 2 decimals. </p>
<p>Divident= 1</p>
<p>Divisor = 4</p>
<p> </p>
Q12:
Determine whether the following are terminating or repeating decimals.
\(\frac{2}{9}\)
Type: Long Difficulty: Easy
<p>=\(\frac{2}{9}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.222\\[-3pt]9\enclose{longdiv}{20}\\[-3pt]\underline{18}\\[-3pt]{20} \\[-3pt]\underline{18}\\[-3pt]\\{20}\\[-3pt]\underline{18}\end{array}\)</p>
<p>Divident = 2</p>
<p>Divisor = 9</p>
<p>Here, \(\frac{2}{9}\) = 0.222 which is repeating decimal. So, it is also a rational number. </p>
<p> </p>
Q13:
Determine whether the following are terminating or repeating decimals.
\(\frac{13}{8}\)
Type: Long Difficulty: Easy
<p>= \(\frac{13}{8}\)</p>
<p>= \(\require{enclose}\begin{array}{r}1. 625\\[-3pt]8\enclose{longdiv}{13}\\[-3pt]\underline{8}\\[-3pt]{50} \\[-3pt]\underline{48}\\[-3pt]\\{20}\\[-3pt]\underline{16}\\[-3pt]{40}\\[-3pt]\underline{40}\\{0}\end{array}\)</p>
<p>Divident = 13</p>
<p>Divisor = 8</p>
<p>Here, \(\frac{13}{8}\) = 1.625 which is terminating decimal.</p>
Q14:
What are the properties of rational numbers?
Type: Short Difficulty: Easy
<ul>
<li>Any rational numbers can be written in a ratio.</li>
<li>It must be divided.</li>
<li>The decimals of rational members are either terminating or recurring. </li>
</ul>
<p> </p>
Q15:
Determine whether the following are terminating or repeating decimals.
\(\frac{1}{8}\)
Type: Long Difficulty: Easy
<p>=\(\frac{1}{8}\)</p>
<p>= \(\require{enclose}\begin{array}{r}0.25\\[-3pt]8\enclose{longdiv}{10}\\[-3pt]\underline{8}\\[-3pt]{20}\\[-3pt]\underline{16}\\[-3pt]{40}\\\underline{40}\end{array}\)</p>
<p>Here, Divident= 1</p>
<p>Divisor = 8</p>
<p>Since, \(\frac{1}{8}\) = 0.25 which is terminating decimal. So, it is rational number. </p>
Videos
Classify Rational Numbers
Add, Subtract, Multiply and Divide Integers
Types of Numbers (Number System)
Rules for Positive and Negative Numbers

Planck’s Radiation Law and Solar Constant
Wein’s law and Rayleigh-jeans law from Planck’s law of radiation
According to plank’s Law we have,
$$E_{\lambda }d\lambda = \frac {8\pi hc}{\lambda ^5}\frac {1}{e^{\frac {hc}{\lambda KT} }-1} d\lambda $$
For shorter wave length \( e^{h}{\lambda KT} \) becomes large compared to unity and hence the Plank’s law reduces to
\begin{align*} E_{\lambda }d\lambda &= \frac {8\pi hc}{\lambda ^5}\frac {1}{e^{\frac {hc}{\lambda KT}}}d\lambda \\ \therefore E_{\lambda }d\lambda &= \frac {8\pi hce^{-\frac {h}{\lambda KT}}}{\lambda^5}d\lambda \\ \end{align*}
which is Wien’s law.
For longerwavelength,
\begin{align*} \therefore E_{\lambda }d\lambda &= \frac {8\pi hc}{\lambda ^5}\frac {1}{1 + \frac {hc}{\lambda KT}+\dots -1}d\lambda \\ E_{\lambda }d\lambda &= \frac {8\pi KT}{\lambda ^4}d\lambda \end{align*}
which is Rayleigh Jeans law. It is clear that Wien’s Law holds for shorter wavelength while Rayleigh Jeans law holds true for longer wavelength.
Deduction of Stefan’s constant from Planck’s Radiation Law
Total radiant energy in unit volume of an isothermal enclosure is
$$ E = \int _0^{\infty } E_{\lambda }\: d\lambda = \int \frac {8\pi hc}{\lambda ^5(e^{hc/ \lambda KT}- 1)}\: d\lambda \dots (1) $$
The total radiant energy in unit volume of an isothermal enclosure is also given by
\begin{align*} E &= AT^4 \dots (2) \\\end{align*}
where A is constant and T is the absolute temperature of enclosure
\begin{align*} \\ AT^4 &= 8\pi hc \int _0^{\infty }\frac {d\lambda }{\lambda ^5} \left (e^{\frac {hc}{\lambda KT}-1}\right )\dots (3) \\ \text {Putting,}\: x= \frac {hc}{\lambda KT} \\ \text {or,}\: \lambda &= \frac {hc}{xKT} \\ \therefore d\lambda &= \frac {-hdx}{x^2KT} \\ \end{align*}
Substituting these value in equation (3) we get \begin{align*}\ \\AT^4 &= 8\pi hc \int _0^{\infty } \frac {\frac {hc}{x^2KT}dx}{\left (\frac {xc}{xKT}\right )^5(e^x -1)} \\ &= \frac {8\pi K^4T^4}{h^3c^3}\int _0^{\infty } \frac {x^3dx}{e^x – 1} \\ \therefore AT^4 &= \frac {8\pi K^4T^4\pi ^4}{15h^3c^3}\:\left [\because \int _0^{\infty }\frac {x^3}{e^x – 1} = \frac {\pi ^4}{15}\right ] \\ \therefore A &= \frac {8\pi K^4\pi ^4}{15h^3c^3} \dots (4) \\ \end{align*}
\begin{align*} \text {Sine Stefan’s constant is given by,} \\ \sigma &= \frac {Ac}{4} \\ \therefore \sigma &= \frac {8\pi ^5 K^4}{15h^3c^3}\frac c4 = \frac {2\pi^5K^4}{15h^3c^2} \\ \end{align*}
Wien’s Constant (b)
According to Wien’s law, Wein’s constant
$$ b = \lambda _{m}T$$
Where \(\lambda _m\) is the wavelength for which the emitted energy is maximum. We have a relation
$$\lambda _m = \frac {hc}{4.965 KT}$$
$$ or, \: \lambda _mT = \frac {hc}{4.965} = 0.2896\: \text {cmK}$$
Solar Constant
Solar constant is defined as the amount of solar energy received per minute by unit area of a perfectly black body placed at a mean distance of the earth from the sun, in absence of the atmosphere and at right angle to the direction of sun’s rays. It is denoted by ‘S’.
Let E be the emissive power of sun, r be its radius. Then the radiant energy emitted by the sun per minute
$$4\pi r^2E\times 60 $$
S be the solar constant, R be the man distance between sun and earth, then the radiant energy absorbed by a perfectly black body having radius R as shown in the figure above is
\begin{align*}&= 4\pi R^2S \dots (2) \\ \text {In the absence of atmosphere,} \\ 4\pi R^2 S &= 4\pi r^2 E \times 60 \dots (3) \\ \text {According to Stefan’s law,}\\ E &= \sigma T^4 \dots (4) \\ \text {From equation}\: (3) and (4)\: \text {we get,} \\ 4\pi R^2 S &= 4\pi r^2 \sigma T^4 \times 60 \\ \text {or,}\: T^4 &= \left ( \frac Rr\right )^2 \frac {S}{60} \times \frac {1}{\sigma } \\ \therefore T &= \left [\left (\frac Rr\right )^2 \frac {S}{60}\times \frac {1}{\sigma } \right ]^{1/4} \dots (5) \\ \end{align*}
Equation (5) represents absolute temperature of sun in terms of Stefan’s constant and solar constant.
Bibliography
S.S. Singhal, J.P. Agarwal, Satya Prakash. heat and thermodynamics and statistical physics. pragati prakashan, 2010.
—. Heat and Thermodynamics and Statistical Physics. Pragati Prakashan, 2010.
Vatsyayan, Dr. Rakesh Ranjan. Refresher Course in Physics. kathmandu: Surya Book Traders, 2015.
Lesson
Black Body Radiation
Subject
Physics
Grade
Bachelor of Science
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