Technical Calculator

Orbital Period Calculator

Enter the required parameters and the calculator will estimate the orbital period instantly.

Satellite Around Central Sphere

Binary System

Orbital period

“The time that an item or satellite tv for pc takes in final touch of 1 whole rotation around some other large item is called the orbital period”

Orbital period Equation:

The system this is used for the low earth orbit is as follows:

\(T = \sqrt(\dfrac{3\pi}{G*P})\)

To calculate the orbital length of a binary star machine, use the subsequent method::

\(T_b=2\pi \sqrt(\dfrac{a^{3}}{G(M_1 + M_2})\)

The way to Calculate Orbital duration?

Go through the subsequent steps to calculate the orbital length::

For Low Earth Orbit:

  • Be aware down the data which you have on paper
  • Multiply 3 through the cost of pi
  • Now multiply the normal gravitational consistent by the suggest density of the imperative frame
  • placed the values within the above-stated orbital duration formulation as we have completed in the following example.

Example:

Suppose the central body density is \(5.51 \, \text{g/cm}^3\), how do we find the orbital period for a low Earth orbit?

Solution:

Given:

  • Density (\(P\)) = \(5.51 \, \text{g/cm}^3\)

Convert density into \(\text{kg/m}^3\):

\[ P = 5.51 \times 1000 \times \left(\frac{1}{100}\right)^3 = 5510 \, \text{kg/m}^3 \]

Gravitational constant (\(G\)):

\[ G = 6.67 \times 10^{-11} \, \text{m}^3 \, \text{kg}^{-1} \, \text{s}^{-2} \]

Orbital period equation:

\[ T = \sqrt{\frac{3 \pi}{G \cdot P}} \]

Substitute the values:

\[ T = \sqrt{\frac{3 \times 3.14159}{(6.67 \times 10^{-11}) \cdot 5510}} \]

Calculate step-by-step:

  • \(3 \times 3.14159 = 9.42477\)
  • \((6.67 \times 10^{-11}) \cdot 5510 = 3.67617 \times 10^{-7}\)
  • \(\frac{9.42477}{3.67617 \times 10^{-7}} = 2.5643 \times 10^{7}\)
  • \(\sqrt{2.5643 \times 10^{7}} = 5063.16 \, \text{seconds}\)

Convert seconds to hours:

\[ T = \frac{5063.16}{3600} \approx 1.406 \, \text{hours} \]

Answer: The orbital period is approximately \(1.406 \, \text{hours}\).

For Binary famous person system:

  • gather the records approximately the applicable parameters together with the semi-fundamental axis, first frame mass, and second frame mass
  • Write down the orbital length formulation
  • positioned the values inside the formula for calculating orbital period as we have completed beneath