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Interstellar space (far from any stars) contains atomic hydrogen (H) with a density of 1 atom/cm3 and at a temperature of about 2.7 K. Determine (a) the pressure in interstellar space, (b) root-mean square speed of the atoms and (c) The kinetic energy stored in 1 km3 of space.

User GwydionFR
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1 Answer

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Step-by-step explanation:

Given that,

Number density
n= 1\ atom/cm^(3) =10^(6)\ atom/m^3

Temperature = 2.7 K

(a). We need to calculate the pressure in interstellar space

Using ideal gas equation


PV=nRT


P=(nRT)/(V)


P=(10^(6)*8.314*2.7)/(6.023*10^(23))


P=3.727*10^(-17)\ Pa


P=36.78*10^(-23)\ atm

The pressure in interstellar space is
36.78*10^(-23)\ atm

(b). We need to calculate the root-mean square speed of the atom

Using formula of rms


v_(rms)=\sqrt{(3RT)/(Nm)}

Put the value into the formula


v_(rms)=\sqrt{(3*8.314*2.7)/(1.007*10^(-3))}


v_(rms)=258.6\ m/s

The root-mean square speed of the atom is 258.6 m/s.

(c). We need to calculate the kinetic energy

Average kinetic energy of atom


E=(3)/(2)kT

Where, k = Boltzmann constant

Put the value into the formula


E=(3)/(2)*1.38*10^(-23)*2.7


E=5.58*10^(-23)\ J

The kinetic energy stored in 1 km³ of space is
5.58*10^(-23)\ J.

Hence, This is the required solution.

User Vivian
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