| To add some back of the napkin calculations to this: Angular resolution of the earth at 66 million light years away would be approximately 2e-17 radians. Using the Raleigh Criterion [0] for lens size for the visible light spectrum (700nm for the best case scenario), you would need a lens with a diameter of about 4e10 meters. That's about the radius of Mercury's orbit around the sun. If you want to see dinosaurs, say 1m resolution, that's about 1.5e-24 radians at 66M light years, needing a lens of diameter 5E17. The entire solar system has a diameter of ~3e14. So even if your lens was the size of the solar system you'd still be off by a factor of 1000 trying to resolve the dinosaurs. At these scales you start running into some pretty fundamental engineering and physics problems with building a telescope this big. Warning: this math may not be totally right, I'm just procrastinating some PDE homework right now, but the scales should be roughly correct. [0] https://en.wikipedia.org/wiki/Angular_resolution#The_Rayleig... |
Probably a mirror rather than a lens. And actually all you need is two mirrors separated by 4e10 meters, not a single mirror of that diameter:
https://en.wikipedia.org/wiki/Astronomical_interferometer
The problem would be the amount of signal you can collect. Might be interesting to do a calculation of the number of photons that would be detectable at that distance per unit solid angle to figure out roughly how big the mirrors would have to be to capture an image in a reasonable amount of time.