00:01
By using the radiation heat transfer coefficient, radiation hit transfer and the stephen bolgman's law, we can write the heat transfer due to radiation, that is q, is equal to p, a, sigma, t2d power of 4 multiplied by time p.
00:23
Or from here, we can write, we can write, emissivity e, emissivity, e is equal to 2 divided by x multiplied by 1 divided by sigma t 2d power 4 so now we can further write e is equal to the value of q can be written as k a t multiplied by t divided by l multiplied by a t whole term multiplied by 1 divided by sigma t 2d power of 4 here k a del t divided by l is the heat transfer due to conductions so from here we get we get e is equal to emissivety is equals to k del t multiplied by 1 divided by l system multiplied by 1 divided by sigma b e2d power of 4 here a a will cancel out each other this will cancel out each other aa will cancel out each other t t t will cancel out each other so let's put the values here we will get amissivity is equal to the value of k we can write the value of k here in this equation is 1 .1 jule per second per meter degree centigrade multiplied by change in temperature.
02:34
Change in temperature is 20 degrees centigrade minus 0 degree centigrade divided where the length is 0 .10 meter multiplied where 1 divided by the value of bulgement constant sigma is 5 .67 multiplied by 10 to the power of minus 8 multiplied by the value of t the temperature here is given 0 degree centigrade that is 0 plus 273 kelvin, 273 kelvin to the power of 4.
03:08
So after solving we get emissivity value e is equals to 220, 220.
03:18
Now directly we will get emissivity is equal to 0 .696, 0 .0 .6.
03:30
So this is the value of emissivity...