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Using Sidereal Time and Geocentric Coordinates



 
 
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Old June 25th 10, 02:44 PM posted to sci.astro
W. eWatson[_2_]
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Default Using Sidereal Time and Geocentric Coordinates

My recent interest in calculating LMST (Local Mean Sidereal Time) came
about from a paper some 30 years old in which the author produce "The
rectangular geocentric systems of coordinates is given by:

X = (R+h)*cos(phi')*cos(LMST)
Y = (R+h)*cos(phi')*sin(LMST)
Z = (R+h)*cos(phi')
where phi' is the geocentric latitude.

I have not found these equations on the web, and am beginning to think
they have been replaced over the decades. Comments?
 




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