S1lent Echoes said:
(Btw, thank you for taking the time to explain such a basic/fundamental concept to/for me, much appreciated)
You’re welcome.
You’re correct – the degree of curvature is greater the closer you get to a mass.
I don’t think anybody knows how mass/energy curves spacetime i.e. what the mechanism is. What Einstein did, though, was give us the mathematical relationship between the mass/energy density in a region and the curvature of spacetime in the neighbourhood. He was struck by a thought: somebody falling freely in the Earth’s gravitational field is completely free of the ordinary effects of the field that we’re familiar with – the feeling of weight. The idea that this effect of gravity could be somehow ‘magicked’ away simply by adopting a different frame of reference to the one we all live in led him to believe the effect of gravity (weight) and the effect somebody in an accelerating object would feel (e.g. a spaceship) were identical (allowing for a few limits). So he pressed on, arriving at the general theory, which allows gravity to be described as the curvature of spacetime.
To explain why time must run more slowly near a mass, I’m going to speak roughly and colloquially. It’s quite long-winded, and won’t please the purists, but it might help. One of the predictions of general relativity is that the radial distance from the centre of a mass to a point on a circle centred on that mass is greater than you’d expect – it’s greater than the circumference of that circle divided by 2∏ (which is what you’d calculate to get the radius of the circle). Somehow, there is more space around a mass than ordinary high-school geometry would suggest. And this effect increases the closer to the mass you get. This is to do with the very curvature of spacetime we’ve been talking about.
Imagine we are located some distance away from a black hole in a circular orbit. We measure the circumference of our orbit to be, say, 6,282 km. So we’d calculate that we must be 1000 km from the centre of the black hole.
We can ascribe a radius to the black hole, which is, let's say, 5km. This would be where its event horizon (the point of no return) is located. Suppose we want to send somebody from our spaceship to hover 3km above its surface, while we stay safely where we are. Ordinarily, we might expect the distance he’d have to travel to be 1000 – 8km = 992km. But in fact, general relativity tells us that, because of the curvature of spacetime, the distance he’d have to cover would be greater than this, say 993km. While I’m just making up these numbers, the principle is quite correct.
So if we aimed a ray of light from our orbiting craft at the black hole, it would have to travel further than we might have expected – it would seem to us to be taking its time to get there. We could only conclude that the light was traveling more slowly than the expected 300,000 km/s. This slowing of light, as measured by us distant observers, is not only allowed by general relativity, but actually predicted by it.
Yet relativity insists that any observer who measures the speed of light locally (i.e. in their immediate neighbourhood) always gets the same value: 300,000 km/s. As the light flashed past our friend, who is hovering just above the black hole, he’d measure its speed to be 300,000 km/s, in accordance with the predictions of relativity.
So we determine the light to be moving ever more slowly as it gets closer to the black hole, yet our hovering shipmate notices nothing unusual about its speed. We can reconcile these two different views only if time for the shipmate is running more slowly than time for us – the slow moving light is moving past him in his slow moving time.