Answer to Question 1
E
Answer to Question 2
Unless the majority of the planets detected are in orbits that we are seeing nearly face on, the objects found are not massive enough to fall into the brown dwarf category. The large number of planets detected by the transit method are in orbits that are nearly edge on, making the minimum mass estimates likely to be fairly close to the actual mass. Many of these have masses much lower than the estimated dividing line between planets and brown dwarfs of about 12 Jupiter masses.