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Estimate the average thermal energy of a helium atom at (i) room temperature (27°C), (ii) the temperature on the surface of the Sun (6000 K), (iii) the temperature of 10 million Kelvin (the typical core temperature in the case of a star).

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The average thermal energy of an atom

is E = 3/2 kBT

where kB = 1.38 x 10-23 JK-1

is the Boltzmann's const.

(i) At room temperature, T = 27°C = 27 + 273 = 300 K

E = 3/2 x 1.38 x 10-23 x 300 = 6.21 x 10-21 J

(ii) At the temperature on the surface of the sun, i.e., T = 6000 K

E = 3/2 x 1.38 x 10-23 x 6000 = 1.24 x 10-19 J

(iii) At T = 10 million Kelvin = 10 x 106 K

E = 3/2 x 1.38 x 10-23 x 10 x 106 = 2.1 x 10-16 J

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