You're confusing linear and angular displacement. These are two separate quantities, which produce their separate effects.
Star trails are due to angular displacement as Earth rotates with some angular velocity. It's what you get when you turn your head around, or stand on a turntable, or at the poles. The dimension of this physical quantity is degrees of angle (or degrees/second for angular velocity).
This has nothing to do with linear displacement caused by linear velocity, such as 'riding' on the Earth's surface or in its orbit around the Sun (but it can be combined with the aforementioned rotational effect - see below).
Linear displacement causes apparent
parallactic motion. This is what you see when riding on a train and looking at closer and father objects passing your visual field at different angular velocities (your visual field is a section of a sphere, centred on you). The magnitude of the parallactic motion is dependent on the distance to the object, and on linear displacement - the closer the object, and the farther you move, the greater the observable parallax.
When you stand on Earth anywhere other than the poles, you are being both rotated and displaced. In a single 12h night (i.e. at equinox) you rotate by 180 degrees and you're displaced by the length of Earth's diameter. Additionally, as you ride the planet in its orbit, you are furthermore and independent from the above displaced by some 1.3 million km, which is obviously more than the Earth's diameter.
So, you've got three observable effects acting at the same time, in the order of their decreasing magnitude:
- angular displacement of the stars due to Earth's rotation making you look in different directions,
- angular displacement due to the parallax caused by being linearly displaced by Earth's orbit,
- angular displacement due to the parallax caused by being linearly displaced by Earth's surface.
Since the latter two depend on the proportion between the distance traveled and the distance to the star (so, are different in magnitude for each star), and this proportion is a very small number even for the closest stars, you won't notice them unless using very precise equipment.