Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Problem 5.19 A sea-level tracking station at latitude +29 makes the following observations of a satel-
lite at the given times.
Topocentric Topocentric
Time Local sidereal time Right ascension Declination
(min) (degrees) (degrees) (degrees)
0.0 90 15.0394 20.7487
1.0 90.2507 25.7539 30.1410
2.0 90.5014 48.6055 43.8910
Use the Gauss method without iterative improvement to estimate the state vector of the satellite.
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Problem 5.20 Refine the estimate in the previous problem using iterative improvement.
Problem 5.21 Calculate the orbital elements from the state vector obtained in the previous problem.
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Problem 5.22 The position vector
R
of a tracking station and the direction cosine vector
ˆ
of a satellite
relative to the tracking station at three times are as follows:
t10 min
R1 1825.96ˆ
I3583.66ˆ
J4933.54 ˆ
K km
 
ˆ
1 0.301687ˆ
I0.200673ˆ
J0.932049 ˆ
K
t21 min
R2 1816.30ˆ
I3575.63ˆ
J4933.54 ˆ
K km
 
ˆ
2 0.793090ˆ
I0.210324ˆ
J0.571640 ˆ
K
t32 min
R3 1857.25ˆ
I3567.54ˆ
J4933.54 ˆ
K km
 
ˆ
3 0.873085ˆ
I0.362969ˆ
J0.325539 ˆ
K
Use the Gauss method without iterative improvement to estimate the state vector of the satellite at the
central observation time.
฀
฀
฀
฀
฀
฀
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Problem 5.23 Refine the estimate in the previous problem using iterative improvement.
Problem 5.24 Calculate the orbital elements from the state vector obtained in the previous problem.
Solutions Manual Orbital Mechanics for Engineering Students Third Edition Chapter 5
Problem 5.25 A tracking station at latitude 60°N and 500m elevation obtains the following data:
Topocentric Topocentric
Time Local sidereal time Right ascension Declination
(min) (degrees) (degrees) (degrees)
0.0 150 157.783 24.2403
5.0 151.253 159.221 27.2993
10.0 152.507 160.526 29.8982
Use the Gauss method without iterative improvement to estimate the state vector of the satellite.
% ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~