The formula to calculate the Orbital Distance (D) is:
\[ D = (P^2)^{1/3} \]
Where:
Orbital Distance (D) is the average distance between an orbiting object and the body it orbits, measured in astronomical units (AU). It is calculated by squaring the orbital period and then taking the cube root of the result. This metric is useful in astronomy to understand the scale of orbits in our solar system and beyond.
Let's assume the following value:
Step 1: Square the period of orbit:
\[ 8^2 = 64 \]
Step 2: Take the cube root of the result:
\[ 64^{1/3} \approx 4 \]
The Orbital Distance (D) is approximately 4 AU.
