The Sun Controls the Solar System
In this activity, you will calculate one powerful quantity, GMsun, and then use it to compute orbital speed, orbit size, and orbital period for Mercury, Earth, and Neptune. Enter only numerical answers in the boxes below.
Newton’s gravitational constant:
Mass of the Sun:
Task: Compute GM_sun = G × M_sun
GMsun = m³/s²
No decimals unless the number is less than 1.
| Planet | Distance from Sun r (m) | Orbital Velocity v (m/s) | Orbit Size 2πr (m) | Period T (s) | Period (years) |
|---|---|---|---|---|---|
| Mercury | 5.79 × 10^10 | ||||
| Earth | 1.496 × 10^11 | ||||
| Neptune | 4.495 × 10^12 |