fresh_42 said:
one emits radiation that can be examined, and the other one does not
I think this is a very simplistic view.
Even if the event horizon of Sag A (assuming that Sag A is in fact a true black hole with a true event horizon) does not itself emit radiation, objects outside the horizon can and do. The reason astronomers believe Sag A is a black hole is that they have observed radiation emitted by objects orbiting it, and have calculated from those observations both the mass of Sag A and the approximate volume of the region of space that it occupies, and the only objects allowed by our best current physical theories that can fit that much mass into that small a volume are a black hole, and the various more exotic solutions that look from the outside like black holes (but don't have true event horizons). In other words, Sag A
can't be a normal star, or a cluster of stars, or a cluster of white dwarfs or neutron stars, etc., etc., etc. None of those things can cram that much mass into that small a space.
Of course we have no way of getting direct evidence that Sag A has a true horizon, if it does. And even if it doesn't, if it turns out to be one of those other more exotic things, we won't be able to tell the difference for a time roughly equal to the Hawking evaporation time for a black hole of the mass of Sag A, which is something like ##10^{90}## years. So even in the case where it would be possible in principle to get direct evidence from inside Sag A, it won't happen for a looooooooooooooooooooooooooooooooooong time. Which means that we won't know for sure about the thing that you say makes such a big difference, for that same amount of time.
To you, that appears to mean that we have to just throw up our hands and wait. To me, it means the thing you say makes such a big difference, doesn't. It doesn't make any practical difference to our ability to do physics.