To get the right answers, you must first ask the proper question. I started this journey wanting to know about relativity. After years of reading through pop science bafflegarble, I started gaining an understanding of the actual issues. After years of that, and many false starts, I finally came to understand that the true question, apparently unasked by science, was “What is motion?”
You’d think such a simple, fundamental question would have been asked and answered decades if not centuries ago. You would be incorrect. Scientists have asked and answered the questions “How do objects move?” and “Why does motion change?” But the central question remained. What is motion in and of itself? What causes it? What is the mechanism?
The answer, like many things in science, to be at once quite simple and devilishly complex. Motion is caused by a gradient in the potential energy field. A gradient in the field causes a self-perpetuating gradient in a particle. The particle’s energy causes gradients in the field.
We interpret the gradient’s velocity at any point by taking the sine of the angle compared to the flat spacetime of the horizontal axis. 0 degrees is stationary (sin 0° = 0). 90 degrees is the speed of light (sin 90° = 1).
But what does that really mean? What is velocity but motion in a direction at a speed? How does the speed of light enter into this?
Velocity, speed, motion, they’re all essentially the same thing: change in distance per change in time. Distance and time. Time and distance. Wait - doesn’t the gradient also have something to say about distance and time?
Indeed it does. The cosine of the gradient’s angle gives the contraction of both space and time. They are always balanced so that the speed of light remains a constant 1. But so what? Why is this important?
Distance is time. Time is distance. It’s not space or time, it’s space and time. Spacetime.
The speed of light, 299,792,458 meters per second, is a conversion factor.
When you are sitting still reading this, you are still moving through time at the rate of one second per second. (We’ll ignore the earth’s rotation, etc.) The gravitational force near the earth’s surface (the angle of the curve) is approximately 9.8 meters per second per second. How much of that is due to motion through space, and how much is motion through time? (Remember, your subjective motion through time is not your objective motion through time.)
Well, you’re not moving (relatively speaking), so all of it is due to the time factor.
That figure of 9.8 meters per second is entirely due to the temporal gradient. None of it is due to the spacial gradient. Even if you were falling instead of sitting still, the spacial gradient is so small as to be nearly irrelevant. 9.8 divided by 299,792,458 is about 0.000,000,003. In the course of normal existence, you can’t tell the difference between that and nothing. It’s lost in the weeds.
Newtonian mechanics works very well in normal, every-day situations.
Relativistic mechanics is for when you can’t ignore the tiny difference. It’s even more important when you are moving so quickly, or being accelerated so strongly, that the spacial component is no longer tiny.
Light from a distant star passing close to the sun is shifted by twice the amount Newton predicted. This is because light travels at, well, the speed of light, so the spacial effects equal the temporal effects. Plus, with radio telescopes, we can measure this effect rather precisely and very close to the sun.
In general, the spacial effects of a force are important if the force is either large or exerted over a very long distance and/or time.
The anomalous perihelion of Mercury (43 arc-seconds per century) is another phenomenon explained by general relativity. See also the two body problem.
The differences caused by the finite speed of the propagation of change in the field are also present, but different. You have to account for the direction and speed the sun is traveling around the galaxy and the amount of time its change of position takes to reach an orbiting planet. The curve contracts and steepens before the sun, and extends and flattens behind it.
And then there’s the frame dragging caused by the sun not actually being a point object, but a rather large, not completely spherical, rotating body.
Physics is hard.