Here are the
(1) Temperature tC in Celsius scale can be converted to temperature tF in Fahrenheit scale using the relation
tC/100 = (tF – 32) /180
Remember that the ice point and steam point of water are 32º F and 212º F respectively in the Fahrenheit scale. These
(2) Temperature tC in Celsius scale can be converted to temperature tK in Kelvin scale (absolute scale) using the relation
tC/100 = (tK – 273.15) /100
so that tC = tK – 273.15 or, tK = tC + 273.15.
Often the above relation is written as tK = tC + 273 very nearly.
The above equation follows from the fact that the ice point and steam point of water are 273.15 K and 373.15 K respectively in the Kelvin scale.
A temperature difference of 1º in the Kelvin scale is equal to a temperature difference of 1º in the Celsius scale.
(3) The increase in length (∆ℓ) of a solid on raising its
∆ℓ = α ℓo ∆T where α is the coefficient of linear expansion (linear expansivity) and ℓo is the original length.
(4) The increase in area (∆A) of a solid on raising its
∆A = β Ao ∆T where β is the coefficient of area expansion (area expansivity) and Ao is the original area.
In the case of isotropic homogeneous solids β = 2α
(5) The increase in volume (∆V) of a solid on raising its
∆V = γVo ∆T where γ is the coefficient of volume expansion (volume expansivity) and Vo is the original volume.
In the case of isotropic homogeneous solids γ = 3α
(6) Specific heat capacity (specific heat) C of a substance is the quantity of heat absorbed or rejected by 1 kg of the substance to change the
Therefore, the heat involved in changing the
(7) Molar specific heat of a substance is the quantity of heat absorbed or rejected by 1 mole of the substance to change the
You know that in the case of gases there are two specific heats viz., specific heat at constant volume and specific heat at constant pressure. Similarly there are two molar specific heats viz., molar specific heat at constant volume and molar specific heat at constant pressure. In this context you will find a useful post here.
(8) Heat transfer takes place by three processes viz., conduction, convection and Radiation.
The quantity of heat Q conducted in a time t through a uniform rod of length L and area of cross section A when the ends of the rod are maintained at a temperature difference ∆T is given by
Q = KA (∆T/L) t where K is the thermal conductivity of the material of the rod
[The temperature gradient ∆T/L is often written as ∆T/∆x, replacing L by ∆x, which will be more appropriate in the case of heat conduction through slabs of thickness ∆x].
The rate of transfer of heat by conduction (time rate), H is given by
H = Q/t = KA ∆T/L
According to Stefan’s law the energy (E) radiated per second per unit surface area of a perfectly black body is directly proportional to the 4th power of the absolute temperature of the body:
E α T4
Or, E = σT4 where σ is Stefan’s constant.
So if the temperature is doubled, the energy radiated from the body will become 16 times.
dQ/dt α (T2 – T1) where dQ is the heat lost in a time dt when the temperatures of the body and the surroundings are respectively T2 and T1.
Note that the loss of heat mentioned in
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