How Does an Asteroid's Radius Affect Its Cooling Rate?

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SUMMARY

The discussion centers on calculating the radius (R) of an asteroid with an iron core and a silicate mantle, given specific parameters. The core density is 8000 kg/m³, the mantle density is 3400 kg/m³, and the mantle thickness is 20% of R. The internal temperature (Ti) is maintained at 600K, while the surface temperature (Ts) is 200K. The thermal conductivity of the silicate mantle is 2 W/(m*K), and the goal is to determine R for a cooling rate of 1 K per million years.

PREREQUISITES
  • Understanding of thermal conductivity and heat transfer principles
  • Familiarity with Boltzmann's constant and its application in thermal energy calculations
  • Basic knowledge of density and its implications in material properties
  • Ability to manipulate equations involving temperature gradients and cooling rates
NEXT STEPS
  • Calculate the cooling rate using Fourier's law of heat conduction
  • Explore the relationship between radius and thermal properties in planetary bodies
  • Research the effects of mantle thickness on cooling rates in asteroids
  • Investigate the implications of core temperature stability on asteroid evolution
USEFUL FOR

Students in astrophysics, planetary science researchers, and anyone interested in the thermal dynamics of celestial bodies.

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Consider an asteroid with an iron core (pc = 8000kg/m^3) covered by a thin silicate mantle (pm = 3400kg/m^3) with a thickness of 20% of the radius R of the asteroid. Assume that the internal temperature Ti = 600K is constant throughout the core. The thermal energy of the core is 3*k*Ti per atom(where k is Boltzmann's constant) and assume that the thermal conductivity of the silicate mantle is about kc = 2 W/ (m*K). Ignore the heat capacity of the mantle. If the surface of the asteroid has a temperature of Ts = 200K find the value of R such that the asteroid has a cooling rate of 1 K / 1 million years.

I really don't know where to start with this question. Any help would be appreciated.
 
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i get the exactly same question...

i don't know how to solve it either...

have you already got the answer yet?
if you have, could you give me some hint?
please email me jaywang19880830@gmail.com
 
gotbrackets? said:
Consider an asteroid with an iron core (pc = 8000kg/m^3) covered by a thin silicate mantle (pm = 3400kg/m^3) with a thickness of 20% of the radius R of the asteroid. Assume that the internal temperature Ti = 600K is constant throughout the core. The thermal energy of the core is 3*k*Ti per atom(where k is Boltzmann's constant) and assume that the thermal conductivity of the silicate mantle is about kc = 2 W/ (m*K). Ignore the heat capacity of the mantle. If the surface of the asteroid has a temperature of Ts = 200K find the value of R such that the asteroid has a cooling rate of 1 K / 1 million years.

I really don't know where to start with this question. Any help would be appreciated.

Well, a good start would be to rewrite this homework question as per the homework posting guidelines.
 

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