A black body is at a temperature 300 K. It emits energy at a rate, which is proportional to
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Proportional refers to the relationship between two quantities where one changes in direct or inverse relation to the other. If two variables are proportional, their ratio remains constant. For example, in direct proportionality, when one quantity increases the other increases at a constant rate and vice versa for inverse proportionality.
Class 11 Physics Chapter 10 Thermal Properties of Matter covers topics like temperature heat and specific heat capacity. It explains thermal expansion calorimetry and heat transfer methods such as conduction and convection. The chapter also introduces the laws of thermodynamics and the behavior of gases under different conditions and temperature changes.
The rate of energy emitted by a black body is governed by the Stefan-Boltzmann law, which states that the energy radiated per unit area is proportional to the fourth power of the temperature:
E ∝ T⁴
So, for a black body at a temperature of 300 K, the energy emitted will be proportional to:
The rate of energy emitted by a black body is governed by the Stefan-Boltzmann law, which states that the energy radiated per unit area is proportional to the fourth power of the temperature:
E ∝ T⁴
So, for a black body at a temperature of 300 K, the energy emitted will be proportional to:
300⁴
Thus, the correct answer is: 300⁴
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