Objective: Define average orbital speed from the equation \$v = \frac{2\pi r}{T}\$ where \$r\$ is the average radius of the orbit and \$T\$ is the orbital period; recall and use this equation. 🚀
Think of Earth as a runner on a giant circular track around the Sun. The orbital speed is how fast the runner (Earth) moves along that track. It’s the distance travelled divided by the time taken to complete one lap.
The average speed \$v\$ is calculated with:
\$v = \dfrac{2\pi r}{T}\$
\$v = \dfrac{2\pi \times 149.6\times10^6}{31\,557\,600}\$
| Parameter | Value | Units |
|---|---|---|
| Average radius (\$r\$) | 149.6 million | km |
| Orbital period (\$T\$) | 31 557 600 | s |
| Average speed (\$v\$) | 29.78 | km/s |
Exam Tip: When you see a question about Earth’s orbital speed, remember:
Keep your answer in km/s unless the question asks otherwise. 🌍