Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186

Emeline Bolmont; Sean N. Raymond; Jérémy Leconte; Alexandre Correia; Elisa Quintana

doi:10.1017/S1743921314007832

Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186

Emeline Bolmont, Sean N. Raymond, Jérémy Leconte, Alexandre Correia, Elisa Quintana

Résultats de recherche: Contribution à un journal/une revue › Article › Revue par des pairs

Résumé

A large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.

langue originale	Anglais
Pages (de - à)	58-61
journal	Proceedings of the International Astronomical Union
Volume	9
Numéro de publication	310
Les DOIs	https://doi.org/10.1017/S1743921314007832
Etat de la publication	Publié - 2014
Modification externe	Oui

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10.1017/S1743921314007832

http://adsabs.harvard.edu/abs/2014IAUS..310...58B

Contient cette citation

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title = "Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186",

abstract = "A large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.",

keywords = "Planets and satellites: dynamical evolution and stability, Planet-star interactions, stars: individual (Kepler-62, Kepler-186), methods: N-body simulations",

author = "Emeline Bolmont and Raymond, {Sean N.} and J{\'e}r{\'e}my Leconte and Alexandre Correia and Elisa Quintana",

year = "2014",

doi = "10.1017/S1743921314007832",

language = "English",

volume = "9",

pages = "58--61",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "310",

}

TY - JOUR

T1 - Tidal evolution in multiple planet systems

T2 - application to Kepler-62 and Kepler-186

AU - Bolmont, Emeline

AU - Raymond, Sean N.

AU - Leconte, Jérémy

AU - Correia, Alexandre

AU - Quintana, Elisa

PY - 2014

Y1 - 2014

N2 - A large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.

AB - A large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.

KW - Planets and satellites: dynamical evolution and stability

KW - Planet-star interactions

KW - stars: individual (Kepler-62

KW - Kepler-186)

KW - methods: N-body simulations

U2 - 10.1017/S1743921314007832

DO - 10.1017/S1743921314007832

M3 - Article

SN - 1743-9213

VL - 9

SP - 58

EP - 61

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - 310

ER -

Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186

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