Interaction of an astronaut with the CMB flux

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SUMMARY

The discussion centers on calculating the physical properties of an astronaut modeled as a perfect spherical absorber in relation to the Cosmic Microwave Background (CMB) radiation. The astronaut's mass is given as 60 kg, with a density of 1000 kg/m³, leading to a calculated volume of 0.06 m³ and a radius of 0.242 m. The surface area is computed as approximately 0.735 m², while the energy absorbed from the CMB is incorrectly stated as E=σΤ^4=3.14*10^-6 J, which does not represent energy due to unit inconsistencies. The conversation emphasizes the need for a correct interpretation of thermal radiation and its implications on the astronaut's body temperature.

PREREQUISITES
  • Understanding of spherical volume and surface area calculations
  • Familiarity with the Stefan-Boltzmann law (E=σΤ^4)
  • Knowledge of specific heat capacity (Q = mCΔT)
  • Basic principles of thermal radiation and energy absorption
NEXT STEPS
  • Review the Stefan-Boltzmann law and its applications in thermal physics
  • Study the concept of thermal equilibrium in relation to energy absorption and emission
  • Explore the implications of the Cosmic Microwave Background radiation on temperature calculations
  • Investigate the relationship between mass, density, and specific heat capacity in thermal dynamics
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Students and professionals in physics, particularly those focusing on thermodynamics, astrophysics, and energy transfer in space environments.

astroYEEET
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Homework Statement
Suppose the body of an astronaut is a perfect spherical absorber with mass 𝑚 = 60 kg and the average density and specific thermal conductivity are d = 1000 kg m-3 and 𝐶 = 4200 J kg-1 K-1
a) What is the approximate rate of energy absorption of the
astronaut due to cosmic microwave radiation (CMB)
The spectral energy distribution of CMB can be approximated by T(CMB) = 2,728 K
b) Approximately how many CMB photons per second will the astronaut absorb?
c) In how much time will CMB radiation increase the temperature of the astronaut by Δ𝑇 = 1 K?
Relevant Equations
E=σΤ^4 where c=5,67×10^−8 W/m^2K^4, Maximum frequency distribution h=3KT where K = 1.38x10^-23 j / K, Q = m 𝐶 ΔT where
Q the heat absorbed by a body of mass m causing an increase in its temperature by ΔΤ and 𝐶 constant of the material
From the density and the mass we can find the volume using d=m/v <=> v=0.06 m^3. Since we consider the astronaut a sphere we find his radius using V(sphere)=4/3*π*R^3 =>R=0.242m. Now we can calculate the surface area with the formula A=4πR^2=0.735m^2.
The energy absorbed will be i suppose equal to E=σΤ^4=3.14*10^-6 J.
Could you offer me any ideas and hints on how to continue the solution. Thanks in advance for your help. (If i have done something wrong please inform me)
 
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Welcome to PF!

astroYEEET said:
Homework Statement:: Suppose the body of an astronaut is a perfect spherical absorber with mass 𝑚 = 60 kg and the average density and specific thermal conductivity are d = 1000 kg m-3 and 𝐶 = 4200 J kg-1 K-1
##c## is the specific heat capacity, not the thermal conductivity.

Relevant Equations::
E=σΤ^4 where c=5,67×10^−8 W/m^2K^4
Note that E here cannot represent energy. To see this, what are the overall dimensions (or units) of σΤ4?

Maximum frequency distribution h=3KT where K = 1.38x10^-23 j / K
I'm not sure what you mean by this. Does h represent Planck's constant? If so, the equation h = 3kT cannot be correct since the overall units for each side do not match.

Q = m 𝐶 ΔT where
Q the heat absorbed by a body of mass m causing an increase in its temperature by ΔΤ and 𝐶 constant of the material
Yes. Here, ##c## is the specific heat capacity of the material.

From the density and the mass we can find the volume using d=m/v <=> v=0.06 m^3. Since we consider the astronaut a sphere we find his radius using V(sphere)=4/3*π*R^3 =>R=0.242m. Now we can calculate the surface area with the formula A=4πR^2=0.735m^2.
Looks good (although I get A = .741 m2)

The energy absorbed will be i suppose equal to E=σΤ^4=3.14*10^-6 J.
As noted above, σΤ4 does not give energy.

Could you offer me any ideas and hints on how to continue the solution. Thanks in advance for your help. (If i have done something wrong please inform me)
Once you have the correct physical interpretation of σΤ4, you might see how to proceed. What are the overall units of σΤ4?
 
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It looks like part (c) wants you to completely ignore any thermal radiation emitted by the astronaut's body. If the astronaut is alive, then he will emit much more radiant energy than he will absorb. So, his body would cool rather than heat up. But, I guess you are to assume that the only energy change of the body is due to CMB radiation absorbed.
 
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