Earlier quoted context omitted.
Possibly, but the challenges to do so are immense. Using the sun as a giant gravitational lens seems much more tractable.
Really? I wouldn't think the sun is nearly massive enough to do what would be required here. Stars visible near the edge of the Sun appear in slightly different spots from their actual locations. If there was a distant planet directly behind the Sun whose light were focused back to an image on our side of the Sun, you'd have to get really far back from the Sun to resolve the image, no? And furthermore, it's exceeding…
> you'd have to get really far back from the Sun to resolve the image, no?
Yah, a few hundred AU.
> you are beholden to the orbital mechanics of your viewing satellite as it plods along.
Yah, any mission like this -- interferometry or gravitational lensing -- is going to be super long and hit very few targets.
> Whereas, multi-site telescopes spread across the Earth have already been demonstrated as a feasible technology
Yah, at radio frequency while pinned to a common rock. The wavelength of visible light is hundreds of nanometers and we're talking across massive distances and significant gravity gradients and even relativistic corrections. The "big" space interferometers currently being considered are in the mid-infrared (e.g. longer wavelengths) across baselines of hundreds of meters.
All of these ideas are really hard.