This is because the maximum value for FOV is 120.
If you want to change this, you have to change the parameter MaxFOV in the main-user.cfg.
This is because the maximum value for FOV is 120.
Thanks, Jack. Is there a way for me to use a keystroke to quickly move around and see what's behind me or do I need to drag the frame around?

The question of what happens at black hole event horizons actually has nothing to do with the singularity. You can replace the singularity with a small but not infinitesimal mass and it's still the same. The properties of the event horizon and the environment around the black hole don't care about what the interior is, other than the total mass of it. This is a consequence of Birkhoff's theorem, which you can think of as a general relativistic version of Newton's Shell Theorem. The gravitational field outside of any spherically symmetric mass is equivalent to the same mass condensed to a singularity.
Maybe, but then we need new physics to explain it and a way to test it through observations.
Completely agree, and one of the stumbling blocks is that some of these theories predict a quantization of space-time at very small scales (5 planck lengths in one theory), and we just haven't been able to detect discrete quantities of space-time. Space-time being continuous is what causes the singularity in the first place and if we could just get at a smaller level than what we are technologically capable of at the current time and find discrete units for space-time our singularity problems will be solved. If space-time isn't continuous at 5 planck lengths, for example, there is no singularity because that is the minimum scale for the singularity (and thus density doesn't ever get to infinity in the D=M/V equation since Volume can never become zero.)The question of what happens at black hole event horizons actually has nothing to do with the singularity. You can replace the singularity with a small but not infinitesimal mass and it's still the same. The properties of the event horizon and the environment around the black hole don't care about what the interior is, other than the total mass of it. This is a consequence of Birkhoff's theorem, which you can think of as a general relativistic version of Newton's Shell Theorem. The gravitational field outside of any spherically symmetric mass is equivalent to the same mass condensed to a singularity.
In a similar way, you can describe the properties of charged particles perfectly well by imagining them as singularities in the electric field. You get the correct predictions as long as you don't care what happens arbitrarily close to those points.
With the Big Bang, you get correct predictions as long as you don't go too close to the initial instant of expansion. Our knowledge of physics is still good up to about 10-32 seconds after the Big Bang! What happened before then requires new physics with quantum gravitation, similarly for describing what happens very close to the center of black holes.
Maybe, but then we need new physics to explain it and a way to test it through observations.
In relativity, travelling backwards in time is the equivalent of choosing a space-like (faster than light) path through space-time rather than a time-like (slower than light) path. For certain observers, that path will be backwards in time. (This is basically the inverse argument for why travelling faster than light is impossible. For certain observers, it is equivalent to going backwards in time, and thus introduces causal paradoxes).
One could propose travelling faster than light actually is possible and avoids paradoxes by creating a new timeline, but then we again must explain how that happens and in a way which makes testable predictions.
Are you on top of a city?
Pretty close to NYC (about 25 miles SE of it). I got the landscape to darken by moving my mouse in a circle while the left button was pressed (I was actually trying to straighten my horizon but this happened instead lol.)

This is such a great comment. Many people think that theories get replaced, or that what we think we know now will be irrelevant in the future. But indeed any new model or theory must explain/predict the very same observations that the old ones did. GR reduces to Newton at slow speeds and weak fields, and whatever future theories of Quantum Gravity must do the same.
Thanks!This is such a great comment. Many people think that theories get replaced, or that what we think we know now will be irrelevant in the future. But indeed any new model or theory must explain/predict the very same observations that the old ones did. GR reduces to Newton at slow speeds and weak fields, and whatever future theories of Quantum Gravity must do the same.

Inside the horizon, the radial coordinate (towards the singularity) becomes time-like, and the time coordinate becomes space-like. The effect of this is that the only allowed (time-like) paths that you can take are inward -- towards the singularity. If you want to move outward (or even stay still!), you would have to follow a space-like path, and this is not allowed.