It's been 4.23 parsecs since we last calculated the derivative of a function in a gravitational wave. Today, we're going to tackle it again.
As we all know, in space, the concept of 'space' is relative. And so is 'calculus'. We'll be discussing the finer points of differential geometry on a rotating asteroid.
The implications of a non-Euclidean geometry on the space-time continuum are far-reaching, and we'll explore them all, one tangent at a time.
To infinity and beyond!