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・ Laplace distribution
・ Laplace equation for irrotational flow
・ Laplace expansion
・ Laplace expansion (potential)
・ Laplace formula
・ Laplace functional
・ Laplace invariant
・ Laplace Island
・ Laplace Island (Antarctica)
・ Laplace Island (Western Australia)
・ Laplace limit
・ Laplace no Ma
・ Laplace number
・ Laplace operator
・ Laplace operators in differential geometry
Laplace plane
・ Laplace pressure
・ Laplace principle (large deviations theory)
・ Laplace transform
・ Laplace transform applied to differential equations
・ Laplace's demon
・ Laplace's equation
・ Laplace's law
・ Laplace's method
・ LaPlace, Louisiana
・ Laplace-P
・ LaplacesDemon
・ Laplace–Beltrami operator
・ Laplace–Carson transform
・ Laplace–Runge–Lenz vector


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Laplace plane : ウィキペディア英語版
Laplace plane
The Laplace plane or Laplacian plane of a planetary satellite, named after its discoverer Pierre-Simon Laplace (1749–1827), is a mean or reference plane about whose axis the instantaneous orbital plane of a satellite precesses.
Laplace's name is sometimes applied to the invariable plane, which is the plane perpendicular to a system's mean angular momentum vector, but the two should not be confused.〔S. Tremaine, J. Touma, and F. Namouni (2009). (Satellite dynamics on the Laplace surface ), ''The Astronomical Journal'' 137, 3706–3717.〕 They are equivalent only in the case where all perturbers and resonances are far from the precessing body.
==Definition==
The axis of this Laplace plane is coplanar with, and between, (a) the polar axis of the parent planet's spin, and (b) the orbital axis of the parent planet's orbit around the Sun.〔 The Laplace plane arises because the equatorial oblateness of the parent planet tends to cause the orbit of the satellite to precess around the polar axis of the parent planet's equatorial plane, while the solar perturbations tend to cause the orbit of the satellite to precess around the polar axis of the parent planet's orbital plane around the Sun. The two effects acting together result in an intermediate position for the reference axis for the satellite orbit's precession.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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