54 is the amount of neutrons there would be
Answer:
i. Cv =3R/2
ii. Cp = 5R/2
Explanation:
i. Cv = Molar heat capacity at constant volume
Since the internal energy of the ideal monoatomic gas is U = 3/2RT and Cv = dU/dT
Differentiating U with respect to T, we have
= d(3/2RT)/dT
= 3R/2
ii. Cp - Molar heat capacity at constant pressure
Cp = Cv + R
substituting Cv into the equation, we have
Cp = 3R/2 + R
taking L.C.M
Cp = (3R + 2R)/2
Cp = 5R/2
Answer:
The temperature of star is 5473.87 K
Explanation:
Given:
Energy difference eV
The ratio of number of particle
Degeneracy ratio
From the formula of boltzmann distribution for population levels,
Where boltzmann constant =
K
Therefore, the temperature of star is 5473.87 K
B)comet nuclei are not uniform in composition