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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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The current impact flux on Mars and its seasonal variation
Youngmin JeongAhn,Renu Malhotra +1 more
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Out-of-plane equilibrium points in the photogravitational restricted four-body problem
TL;DR: In this paper, the photogravitational restricted four-body problem is employed to describe the motion of an infinitesimal particle in the vicinity of three finite radiating bodies.
Journal ArticleDOI
WASP-54b, WASP-56b and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP ⋆
Francesca Faedi,Francesca Faedi,Don Pollacco,Don Pollacco,S. C. C. Barros,D. J. A. Brown,A. Collier Cameron,Amanda P. Doyle,R. Enoch,Michaël Gillon,Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Guillaume Hébrard,Guillaume Hébrard,Monika Lendl,C. Liebig,Barry Smalley,Amaury H. M. J. Triaud,Richard G. West,Peter J. Wheatley,Khalid Al-Subai,David R. Anderson,David J. Armstrong,David J. Armstrong,Joao Bento,J. Bochinski,François Bouchy,François Bouchy,R. Busuttil,Luca Fossati,A. Fumel,Carole A. Haswell,Coel Hellier,S. Holmes,Emmanuel Jehin,Ulrich Kolb,James McCormac,James McCormac,Grant Miller,C. Moutou,Andrew Norton,N. R. Parley,Didier Queloz,Alexandre Santerne,Ian Skillen,Alexis M. S. Smith,Stéphane Udry,Christopher A. Watson +48 more
TL;DR: WASP-54b is a sub-Jupiter mass planet of mass 0.636(-0.024)(+0.033)) and radius 1.653 (−0.083)(+ 0.090) R-J as discussed by the authors.
Journal ArticleDOI
Obliquity variations of terrestrial planets in habitable zones
TL;DR: In this paper, the authors investigated the obliquity variations of possible terrestrial planets in habitable zones (HZs) perturbed by a giant planet(s) in extrasolar planetary systems.