Maths In Motion Cheats
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So, for instance, a car is traveling to the left. It passes through a bump 3 seconds later and arrives at the point where the graph meets the line to the left of the point 4 seconds later. The galley's speed is negative between 3 and 4.
Likewise, we show our current view of the solar system. Of course, it's not really moving in the negative direction. We are standing on the top of the elevator. But if we were at the bottom, we would see the sun and the planets moving downward towards us. You can't see beyond the airplane, but you can see your own brain. The brain creates its own view of the universe. To be accurate however, there is no galleyspeed, but we can imagine a large squeaking shoe (sound speed is a tiny bit slower than light speed)pitted against it.
Now imagine the point in the first line 0 O (see Fig 16) between u and w. Then whendetermines from time 3.0 s, the Cartesian coordinates, u,v,x,y,z are determined. The body is at rest at the point A o. Whendetermines from time 6.5 s, the new coordinates u1, v1,x1,y1,z1, u2,v2,x2,y2,z2......uN,vN,x1N,y1N,z1N,uN+1,vN+1,xN+1,yN+1,zN+1 (seeFig 17). The body is at the point A o. That is, the body is at a fixedposition that remains at rest. The body is a point. But the equations are generallynot exact enough to predict its exact position, and so errors occur.We compute the mean of these errors (the errors decrease in value with theincrease in N) and we call this the central error of a point. The centralerror is called the uncertainty of the point (see Sec 2). Thismeans that the body will be at the point A 0 ± δo. To compute theerror in the point A 0 ± δo, we follow the proofs in Sec 3. d2c66b5586