Giant branch planetary systems: Dynamical and radiative evolution

Mustill, Alexander J.

doi:10.1016/b978-0-443-21439-4.00011-0

Reference Module in Materials Science and Materials Engineering 2024

DOI: 10.1016/b978-0-443-21439-4.00011-0

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Giant branch planetary systems: Dynamical and radiative evolution

Alexander J. Mustill

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2024

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Lagrange’s planetary equations with time-dependent secular perturbations

Deme

2024

Celest Mech Dyn Astron

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The long-term evolution of quasi-Keplerian systems is driven by a Hamiltonian that is independent of the fast angle. As this Hamiltonian may contain explicitly time-dependent parameters, the conservation of mechanical energy is not guaranteed in such systems. We derive how the semi-major axis evolves in these cases. We analyze two astrophysically interesting examples, those of the harmonic and quadrupole perturbations.

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Lagrange’s planetary equations with time-dependent secular perturbations

Deme

2024

Celest Mech Dyn Astron

View full text Add to dashboard Cite

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Giant branch planetary systems: Dynamical and radiative evolution

Cited by 1 publication

References 33 publications

Lagrange’s planetary equations with time-dependent secular perturbations

Lagrange’s planetary equations with time-dependent secular perturbations

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