Equations for the Origin of Stellar and Planetary Rotations
POSTER
Abstract
Prior to stellar formation dense stellar cores of hydrogen gas with rotational momentum of $I\omega_{core}$ were orbited by partial rings of hydrogen gas which were in motion with angular momentum of mvr. As gravitational attraction of the rings occurred, the rings of gas decayed and tangentially collided and attached to the stellar cores transfering their angular momentum to the already rotating stellar cores creating final rotation. The equation for this final rotation is $ m_1v_1r_1 +m_2r_2v_2 + m_nv_nr_n + I\omega_{stellar core}= I_{\omega_{star}}$. Planetary formation began with rotating planetary cores of rotational momentum $I\omega_{planetary core}$. These cores were orbited by molten partial rings of compounds such as silicates, carbonates etc which decayed due to gravitational attraction. These rings had orbital angular momentum mvr. The decaying rings attached to the planetary cores tangentially tranfering their angular momentum and mass to the cores creating a final planetary rotation of $m_1v_1v_1 + m_2v_2r_2 +m_nv_nr_n + I\omega_{planetary core} = I\omega_{planet}$.
Authors
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Stewart Brekke
Northeastern Illinois University (former grad student)