01-17-2016, 08:21 AM
To produce radiation at the temperature of the CMBR, the outer shell needs to be many AU wide- especially since this is an F-Class star, brighter than our Sun.
In addition, if it were only a partial dyson, some of the inner layers would surely radiate through the gaps - I can't imagine how to avoid this using any configuration I'm familiar with.
In addition, if it were only a partial dyson, some of the inner layers would surely radiate through the gaps - I can't imagine how to avoid this using any configuration I'm familiar with.