Key Takeaways:
- The Sun exhibits a velocity of 16,000 mph (25,200 km/h) relative to the average rotational motion within the galaxy.
- The Sun's velocity towards the galactic center is measured at 22,000 mph (36,000 km/h).
- A vertical velocity component of 11,000 mph (18,000 km/h) is observed for the Sun's motion within the galaxy.
- These velocities represent the Sun's movement within the galactic context, exceeding the average galactic rotation speed.
Compared to the average motion, the Sun appears to move a little faster — 16,000 mph (25,200 km/h) — than the general rotation. It’s moving toward the galactic center at 22,000 mph (36,000 km/h) and slightly upward at 11,000 mph (18,000 km/h).
