I have been researching the ECAT sized metal spheres in order to determine the 
expected behavior as their diameters are varied.  This has lead to some 
interesting results which I share on occasion with the vortex in the hope that 
the insight will spark ideas within the group.  Whether or not this information 
is helpful is left to the discretion of the readers.

My assumed system consists of 100 grams of nickel generating 10000 watts of 
heat power.  Each reaction releases 5 MeV of energy.  The actual physical 
source of the energy is not taken into consideration since that is not 
generally understood as of this time.

My crude model consists of a very large quantity of nickel spheres of an 
assumed diameter such that the total mass is as listed above.  One of my 
variables is obviously the diameter of each sphere which is modified in an 
attempt to understand what might be expected as this dimension is changed.  For 
the following results I am attempting to estimate the temperature of a single 
sphere in open space that emits all of the energy generated within without 
having any incoming radiation to balance since it sees cold space as it looks 
outward.  In normal operation each sphere will be surrounded by the thermal 
environment so that it must operate at a higher temperature than my calculation 
suggests and that is one of the paths that I am pursuing in further research.  
The calculations that I am posting would therefore represent a low extreme 
temperature value that could not be reduced if the power output constraints are 
to be met.

I chose an emissivity of .8 for the nickel material, but this can be modified 
if anyone has a better estimate and wants me to take it into consideration.  
The radiation from the surface is assumed to be normal to the sphere surface.

I calculate that the temperature of the 10 micrometer diameter test sphere is 
425 K degrees (152 C) in open space.  This is the minimum temperature that the 
surface of the sphere supports which will result in the expected radiation 
level.  If the sphere is surrounded by other spheres or parts of the system at 
an operating temperature that is required to transfer energy to the load by 
radiation the temperature will have to increase in order to deposit its portion 
of the total energy.   Conduction and convection are not taken into 
consideration for this calculation.

The absolute surface temperature of each sphere must increase as the diameters 
increase.  This is not too surprising since the total surface area of the large 
collection of spheres is reduced as the diameter of each sphere increases.  
Since the power is assumed constrained at 10000 watts the surface power density 
by necessity must rise.  My model was tested with varying diameters of spheres 
and the relationship appears to follow an interesting function.  It so happens 
that the absolute temperature is directly proportional to the forth root of the 
diameter ratio.  To clarify the calculation, you take the desired sphere 
diameter and divide it by the original diameter first.  Then take this ratio 
and raise it to the .25 power.  The result will be the absolute temperature 
ratio expected for radiation of a constant total power.

In the case that I use as reference you would obtain: initial 10 micrometer 
sphere collection, with absolute temperature of 425 K: desired 160 micrometer 
diameter spheres.  Calculate 160 micrometers/10 micrometers = 16.   Take the 
forth root of 16 and obtain 2.  Since the 10 micrometer spheres reach 425 K, 
the 160 micrometer spheres should be at 850 K (578 C) as the calculated value.  
The numbers are rounded for clarity.

Dave


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