Mr Spinkles
Mr
Well said, however the fact that we need four coordinates (x,y,z,t) to locate an event was true in classical physics before Einstein, this goes back to Galileo and is called Galilean relativity.fantome profane said:Ok, moving on. 4 dimensional spacetime consists of 3 dimensions of space plus one dimension of time. Lets imagine that you and I decide to meet somewhere in New York City. So how many points of information would you have to give me (or I give you) to insure that we do actually meet? Well you could give me the location that you intend to meet me, the longitude(1) and latitude(2) and since New York contains many tall buildings you might also have to tell me what floor to go to – height(3). So there are three coordinates that refer to the three dimensions of space. But obviously this is not enough information, you will also have to tell me what time(4) you want to meet. So there you have time being the fourth dimension of spacetime. Every point in our four dimensional universe* can be defined by four coordinates.
In this case, the "normal" case we are all intuitively familiar with, x,y,z,t in one reference frame S is related to x',y',z',t' of another reference frame S' in a simple and intuitive way. E.g. if the reference frames are at rest relative to each other, and they are oriented the same way, and they are separated by a distance X along their x-axes, then x' = x + X. Of course if the reference frames are moving relative to each other and accelerating and rotating, the equations may not seem so "simple" but you can nevertheless figure it out, step by step, using your intuition of the geometry of space and drawing pictures.
We are all familiar with the consequences of Galilean relativity. For example two racecars that are neck-and-neck may be going 100 mph, around in circles, in a reference frame fixed to the grandstand. However, in a reference frame fixed to one of the racecars, both racecars are stationary and separated by a small distance and the grandstand is going around in circles.
Another example: the length of some object is always the same in a Galilean (intuitive) reference frame even if they are moving relative to each other in complex ways.
The counter-intuitive thing about Einstein's Relativity is that the coordinates x,y,z,t in one reference frame are mixed up, and related in a strange way to the coordinates x',y',z',t' in a different reference frame. This is one thing that was truly different about Relativity, and it leads to conceptually bizarre consequences that you would be very unlikely to work out by drawing diagrams and using your intuition.
Here's one striking example of relativity, the curvature of space at large scales causes the light from galaxies in this deep space photo to be distorted. Galaxy Cluster Abell 1689