The Earth is a moving object in space; it is never at rest.
The Earth completes a full 360° rotation on its axis every day.
This results in a speed at the equator of roughly 1700 km/hr, which decreases as you move toward the poles.
Simultaneously, Earth orbits the Sun at speeds between 29.29 km/s and 30.29 km/s.
The fastest speeds occur in early January at perihelion, while the slowest are in July at aphelion.
Beyond that, the Solar System itself moves through the Milky Way.
Our speed relative to the Sun is between 200 and 220 km/s, inclined at about 60° to the plane of the planets.
This motion isn’t a vortex but simply the sum of these velocities.
On a larger scale, the Milky Way and Andromeda galaxies are moving toward each other at 109 km/s.
Gravitational forces from both dense and less dense regions influence the motion of our Local Group.
Altogether, we are moving at 627 ± 22 km/s relative to the universe’s average.
However, the leftover photons from the Big Bang provide a unique cosmic frame of reference.
The Sun moves at a total speed of 368 km/s relative to the Cosmic Microwave Background (CMB).
There is an uncertainty of ± 2 km/s due to not knowing the exact magnitude of the CMB dipole.
Given our location within the Milky Way, we can only speculate about taking these kinds of measurements.
It’s the Earth’s south pole that points toward the center of the Milky Way.
You have it backwards in your main photo at the top of the page.