Equatorial bulge: Difference between revisions

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|bibcode=2011PhRvD..84l4001I
|doi=10.1103/PhysRevD.84.124001
|s2cid=118305813
}}</ref><ref>{{cite journal
|last1=Renzetti
|first1=G.
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|bibcode=2013JApA...34..341R
|doi=10.1007/s12036-013-9186-4
|s2cid=120030309
}}</ref><ref>{{cite journal
|last1=Renzetti
|first1=G.
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|bibcode=2014Ap&SS.352..493R
|doi=10.1007/s10509-014-1915-x
|s2cid=119537102
}}</ref> They depend on the orientation of the Earth's symmetry axis in the inertial space, and, in the general case, affect ''all'' the Keplerian [[orbital elements]] with the exception of the [[semimajor axis]]. If the reference ''z'' axis of the coordinate system adopted is aligned along the Earth's symmetry axis, then only the [[longitude of the ascending node]] Ω, the [[argument of pericenter]] ω and the [[mean anomaly]] ''M'' undergo secular precessions.<ref>{{cite journal
|last1=King-Hele
|first1=D. G.