outandbeyond2004
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Second part of a three-part post
Wrt a particular rf attached to the rl,
\vec P_L = R_L(cos\phi, sin\phi, 0)
where \phi = \phi_0 at time t = 0.
If we orient a reference frame attached to the planet (rfP) so that its z axis runs through \vec\omega_e and the angle from \vec\omega_e to \vec P_p is \theta_p, then wrt rfP
\vec P_L = R_L(cos\theta_p cos\phi, sin\phi, -sin\theta_p cos\phi) + \vec P_p
Let us orient a reference frame attached to ether space (rfE) so that its x-axis runs through \vec v_e and its y-axis points in the direction of \vec \omega_e \times \vec v_e . Let the angle from the z axis to the angular velocity be \theta_e . Then wrt rfE,
\vec P_L = R_L( (cos\theta_e cos\theta_p - sin\theta_e sin\theta_p)cos\phi,
sin\phi,
-(sin\theta_e cos\theta_p + cos\theta_e sin\theta_p)cos\phi )
+ \vec P_p + \vec P_e
where \vec P_e is the position of the planet's center wrt rfE.
Wrt a particular rf attached to the rl,
\vec P_L = R_L(cos\phi, sin\phi, 0)
where \phi = \phi_0 at time t = 0.
If we orient a reference frame attached to the planet (rfP) so that its z axis runs through \vec\omega_e and the angle from \vec\omega_e to \vec P_p is \theta_p, then wrt rfP
\vec P_L = R_L(cos\theta_p cos\phi, sin\phi, -sin\theta_p cos\phi) + \vec P_p
Let us orient a reference frame attached to ether space (rfE) so that its x-axis runs through \vec v_e and its y-axis points in the direction of \vec \omega_e \times \vec v_e . Let the angle from the z axis to the angular velocity be \theta_e . Then wrt rfE,
\vec P_L = R_L( (cos\theta_e cos\theta_p - sin\theta_e sin\theta_p)cos\phi,
sin\phi,
-(sin\theta_e cos\theta_p + cos\theta_e sin\theta_p)cos\phi )
+ \vec P_p + \vec P_e
where \vec P_e is the position of the planet's center wrt rfE.
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