- What is Planckâs equation?
- Planckâs constant
- Planckâs Law of the equation
- Planckâs Equation for Class 12
- Illustrated Examples
- FAQs on Planckâs Equation
What is Planckâs equation?
Planck's law can be defined as the density of electromagnetic radiations produced at a temperature by a dark body in thermal equilibrium. The radiations emit the energy between the environment and body is zero or null. In the last years of the 19th century, it was difficult for physicists to understand the sudden rise in frequencies in the spectrum of black body radiations.Â
The energy in Planckâs equation is transferred as quanta and is denoted as H. The value of H is 6.63 x 10-34 J/s. When the frequency of a photon is clear or precise, then the energy of a photon can be calculated with the help of Planckâs law.Â
Planckâs constant
Planckâs constant is the relevance between the relationship of electromagnetic radiation of the frequency and the energy of a quantum.Â
The equation of the Planck isÂ
E = hv
Here, v is the frequency of the radiation.
V can also be denoted as f
H is the Planckâs constant, the value of h = 6.63 x 10-34 J/s
Planckâs Law of the equation
The Planck law states the electromagnetic radiations released from the bodies are notÂ
released in a continuous manner. It is made up of quanta denoted as h, and the size of Planckâs constant.Â
It can be written asÂ
| B Îğ (T) = 2hc2 / Îğ5. 1 / hc / ekt Îğ â 1 |
Here, h is the Planckâs constant which is equal to 6.63 x 10-34 J/s
K is the Boltzmannâs constant which is equal to 1.381 x 10-23 J/K
The released emissionsâ wavelength is inversely proportional to the frequency. it can be written as Îğ = c/v.
Explanation
The temperature of the blackbody can go up to hundreds of degrees. Most of the radiations in the electromagnetic spectrum are infrared radiations. The total radiated energy increases with the increase in temperature. Likewise, the total radiated energy decreases with a decrease in temperature. When temperature increases, the release shifts in the spectrum cause the wavelengths to go short. It causes visible light which is a significant part of the radiation.Â
Planckâs Equation for Class 12
The chapter on electromagnetism holds a weightage of 3 marks. These 3 marks contain one very short question of 1 mark and one short question of 2 marks.
Illustrated Examples
Example 1: Write down the equation for the released emission.
Answer: The released emissionsâ wavelength is inversely proportional to the frequency. it can be written as Îğ = c/v.
Example 2: Write down Planckâs law of equation.Â
Answer: It is made up of quanta denoted as h and the size of Planckâs constant. It can be defined as follows âÂ
B Îğ (T) = 2hc2 / Îğ5. 1 / hc / ekt Îğ â 1
Example 3: Explain the relation between Planckâs constant and a photonâs energy?
Answer:Â When the frequency of a photon is clear or precise, then the energy of a photon can be calculated with the help of Planckâs law.
FAQs on Planckâs Equation
Q: In Planckâs equation, whatâs the amount of energy emitted by radiation?
Q: What is H in Planckâs equation?
Q: What do you understand by Planckâs constant?
Q: What do you mean by Planckâs law of equation?
Q: Whatâs the value of Boltzmannâs constant?
Physics Electromagnetic Induction Exam
Student Forum
Other Topics under this Chapter
- Experiments of Faraday and Henry
- Motional Electromotive Force
- Combination of Capacitors
- Parallel Plate Capacitor
- Electrostatics of Conductors
- Electromagnetism
- Torque on current loop, magnetic loop dipole
- Moving Coil Galvanometer
- Force between two parallel currents, the Ampere
- The Solenoid and the Toroid
- Magnetic Force
- Planck Equation
- Curie Weiss Law
- Electromotive Force
- Magnetic Effect of Electric Current
Other Class 12th Physics Chapters
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- Physics Magnetism and Matter
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