Quote:
Originally Posted by timb
Ok, I was slow too this morning. I think Fomalhaut b was quite a good deal brighter in the optical (600nm) than you calculated. The discovery paper tried to explain this by suggesting the Fomalhaut-light was reflecting off a large circumplanetary disk.
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Thanks for the paper. I had seen one article saying the 20 to 40 Jupiter radii for the object might be due to moons. The circumplanetary disk seems to be the better answer and the paper states it to be 100x brighter than if it were a Jupiter size object. That seems to put the exoplanet at a 22.5 magnitude.