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Solar system dynamics
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In this paper, the two-body problem and the restricted three body problem are considered. And the disturbing function is extended to include the spin-orbit coupling and the resonance perturbations.Abstract:
Preface 1 Structure of the solar system 2 The two-body problem 3 The restricted three-body problem 4 Tides, rotation and shape 5 Spin-orbit coupling 6 The disturbing function 7 Secular perturbations 8 Resonant perturbations 9 Chaos and long-term evolution 10 Planetary rings Appendix A Solar system data Appendix B Expansion of the disturbing function Indexread more
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Near-Infrared Coronagraphy of the GG Tauri A Binary System
Yoichi Itoh,Motohide Tamura,Saeko S. Hayashi,Yumiko Oasa,Misato Fukagawa,Norio Kaifu,Hiroshi Suto,Koji Murakawa,Yoshiyuki Doi,Noboru Ebizuka,Takahiro Naoi,Hideki Takami,Naruhisa Takato,Wolfgang Gaessler,Tomio Kanzawa,Yutaka Hayano,Yukiko Kamata,D. Saint-Jacques,Masanori Iye +18 more
TL;DR: In this article, the GG Tau A binary system was obtained with the Coronagraphic Imager with Adaptive Optics (CIAO) mounted on the Subaru Telescope and the images showed that its circumbinary disk is smooth and does not have 0. 1 scale structures.
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How common are Earth–Moon planetary systems?
TL;DR: Morishima et al. as discussed by the authors show that massive moons orbiting terrestrial planets are not rare and that giant impacts with the required energy and orbital parameters for producing a binary planetary system do occur with more than 1 in 12 terrestrial planets hosting a massive moon.
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Planetary migration and eccentricity and inclination resonances in extrasolar planetary systems
TL;DR: In this article, it was shown that the 2:1 eccentricity-type mean-motion resonances are sensitive to the migration rate within the range expected for type II migration due to planet-disk interaction.
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Modelling the KIC8462852 light curves: Compatibility of the dips and secular dimming with an exocomet interpretation
TL;DR: In this paper, the authors show how the dips and secular dimming in the KIC8462852 light curve can originate in circumstellar material distributed around a single elliptical orbit (e.g. exocomets).
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Rotation Period Evolution in Low-mass Binary Stars: The Impact of Tidal Torques and Magnetic Braking
TL;DR: In this paper, the authors examined how tides, stellar evolution, and magnetic braking shape the rotation period (P$_{rot}$) evolution of low-mass stellar binaries up to orbital periods (p$_{orb}$), across a wide range of tidal dissipation parameters using two common equilibrium tidal models.