Nominal Mean Motion Solution

STEP 0: Pre-Calculation Summary
Formula Used
Nominal Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3)
no = sqrt([GM.Earth]/asemi^3)
This formula uses 1 Constants, 1 Functions, 2 Variables
Constants Used
[GM.Earth] - Earth’s Geocentric Gravitational Constant Value Taken As 3.986004418E+14
Functions Used
sqrt - A square root function is a function that takes a non-negative number as an input and returns the square root of the given input number., sqrt(Number)
Variables Used
Nominal Mean Motion - (Measured in Radian per Second) - Nominal Mean Motion refers to the average rate at which a satellite orbits around a celestial body, such as the Earth.
Semi Major Axis - (Measured in Meter) - The Semi major axis can be used to determine the size of satellite's orbit. It is half of the major axis.
STEP 1: Convert Input(s) to Base Unit
Semi Major Axis: 581.7 Kilometer --> 581700 Meter (Check conversion ​here)
STEP 2: Evaluate Formula
Substituting Input Values in Formula
no = sqrt([GM.Earth]/asemi^3) --> sqrt([GM.Earth]/581700^3)
Evaluating ... ...
no = 0.0450008059755109
STEP 3: Convert Result to Output's Unit
0.0450008059755109 Radian per Second --> No Conversion Required
FINAL ANSWER
0.0450008059755109 0.045001 Radian per Second <-- Nominal Mean Motion
(Calculation completed in 00.004 seconds)

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Created by Shobhit Dimri
Bipin Tripathi Kumaon Institute of Technology (BTKIT), Dwarahat
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Satellite Orbital Characteristics Calculators

Mean Anomaly
​ LaTeX ​ Go Mean Anomaly = Eccentric Anomaly-Eccentricity*sin(Eccentric Anomaly)
Mean Motion of Satellite
​ LaTeX ​ Go Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3)
Local Sidereal Time
​ LaTeX ​ Go Local Sidereal Time = Greenwich Sidereal Time+East Longitude
Anomalistic Period
​ LaTeX ​ Go Anomalistic Period = (2*pi)/Mean Motion

Nominal Mean Motion Formula

​LaTeX ​Go
Nominal Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3)
no = sqrt([GM.Earth]/asemi^3)

What does orbital motion mean?

Orbital Motion refers to the movement of a satellite around a celestial body, such as the Earth, following a specific path known as an orbit.

How to Calculate Nominal Mean Motion?

Nominal Mean Motion calculator uses Nominal Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3) to calculate the Nominal Mean Motion, The Nominal Mean Motion formula is defined as the angular speed required for a body to complete one orbit, assuming constant speed in a circular orbit which completes in the same time as the variable speed, elliptical orbit of the actual body. Nominal Mean Motion is denoted by no symbol.

How to calculate Nominal Mean Motion using this online calculator? To use this online calculator for Nominal Mean Motion, enter Semi Major Axis (asemi) and hit the calculate button. Here is how the Nominal Mean Motion calculation can be explained with given input values -> 4.7E-6 = sqrt([GM.Earth]/581700^3).

FAQ

What is Nominal Mean Motion?
The Nominal Mean Motion formula is defined as the angular speed required for a body to complete one orbit, assuming constant speed in a circular orbit which completes in the same time as the variable speed, elliptical orbit of the actual body and is represented as no = sqrt([GM.Earth]/asemi^3) or Nominal Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3). The Semi major axis can be used to determine the size of satellite's orbit. It is half of the major axis.
How to calculate Nominal Mean Motion?
The Nominal Mean Motion formula is defined as the angular speed required for a body to complete one orbit, assuming constant speed in a circular orbit which completes in the same time as the variable speed, elliptical orbit of the actual body is calculated using Nominal Mean Motion = sqrt([GM.Earth]/Semi Major Axis^3). To calculate Nominal Mean Motion, you need Semi Major Axis (asemi). With our tool, you need to enter the respective value for Semi Major Axis and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
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