STEP 3: FINDING THE MEAN ANOMALY

M



 
Element Symbol Value
Epoch to 05:54:21.171 UTC December 16, 2007
Inclination i 51o.9970
R.A. of the Ascending Node aW0 251o.0219
Eccentricity e 0.0001492
Argument of Perigee w0 33o.8641
Mean Anomaly at TLE Epoch Mo 326o.2322
Mean Motion n 12.62256095 orbits / solar day
Propagation Time Dt 1.7677141 solar days


The satellite's Mean Anomaly at the chosen time t is determined using the following equation:

M(t) = Mo + 360o { nDt - INT(nDt) - INT[ [ Mo+360o( nDt - INT(nDt) ) ] / 360o ] }

M(t) = 78o.940629

This equation ensures that the determined Mean Anomaly always lies between 0 and 360 degrees.

To proceed to the next step, the Mean Anomaly must first be expressed in terms of radians by using the following equation:

M(t) (radians) = [ M(t) (degrees) ] [ p / 180o ]

 M(t) = 1.37777389 radians

 

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Step 3: Finding the Mean Anomaly Was Last Modified On January 02, 2012