Calculating Dust Particle Size in Solar System Orbit - Electromagnetism Help

In summary, the conversation discusses the calculation of the time average poynting vector of radiation at a given distance from the sun, using the sun's total luminosity and the properties of dust particles in the solar system. The conversation also mentions estimating the maximum size of a dust particle that can remain in orbit around the sun without being blown away by radiation pressure. The use of the Poynting vector and the luminosity equation is suggested to solve these calculations.
  • #1
andyfreesty1e
14
0
urgent electromagnetism help

Homework Statement


Assume that dust particle in the solar system are spherical, black and have a density of 2000kg/m^3. Use the total luminosity of the sun to calculate the time average poynting vector of the radiation at a distance r from the Sun. Hence estimate what is the maximum size of a dust particle that can be help in orbit by gravity around the sun without being blown away by radiation pressure.


Homework Equations




The Attempt at a Solution


I have no idea about finding the poynting vector

For the second bit do i use P=F/A and F=GMm/R^2, and P(radiation)=S/c?
 
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  • #2


If you use the luminosity equation I=P/A you don't need to work out the pointing vector. The P value from the previous equation will give you that.

For your own info P=[HxE] is the Poynting vector.
 

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