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相关论文: Secular Evolution of Planetary Systems in Binaries

200 篇论文

In this letter we consider the evolution of a planetary system around a star inside a wide binary. We simulate numerically the evolution of the planetary orbits for both co-planar and highly-inclined systems. We find that the Kozai…

天体物理学 · 物理学 2008-11-26 Daniel Malmberg , Melvyn B. Davies , John E. Chambers

One of the most remarkable properties of extrasolar planets is their high orbital eccentricities. Observations have shown that at least 20% of these planets, including some with particularly high eccentricities, are orbiting a component of…

天体物理学 · 物理学 2009-11-10 G. Takeda , F. A. Rasio

Many recent observational studies have concluded that planetary systems commonly exist in multiple-star systems. At least ~20%, and presumably a larger fraction of the known extrasolar planetary systems are associated with one or more…

天体物理学 · 物理学 2009-11-13 Genya Takeda , Ryosuke Kita , Frederic A. Rasio

Many recent observational studies have concluded that planetary systems commonly exist in multiple-star systems. At least ~20% of the known extrasolar planetary systems are associated with one or more stellar companions. The orbits of…

天体物理学 · 物理学 2009-11-13 Genya Takeda , Ryosuke Kita , Frederic A. Rasio

The most puzzling property of the extrasolar planets discovered by recent radial velocity surveys is their high orbital eccentricities, which are very difficult to explain within our current theoretical paradigm for planet formation.…

天体物理学 · 物理学 2009-11-11 Genya Takeda , Frederic A. Rasio

Planets have been observed in tight binary systems with separations less than 20 AU. A likely formation scenario for such systems involves a dynamical capture, after which high relative inclinations are likely and may lead to Kozai…

地球与行星天体物理 · 物理学 2011-02-11 Lamya Saleh , Frederic Rasio

We investigate the orbital dynamics of circumbinary planetary systems with two planets around a circular or eccentric orbit binary. The orbits of the two planet are initially circular and coplanar to each other, but misaligned with respect…

地球与行星天体物理 · 物理学 2021-12-15 Cheng Chen , Stephen H. Lubow , Rebecca G. Martin

We examine the effects of dynamical evolution in clusters on planetary systems or protoplanetary disks orbiting the components of binary stars. In particular, we look for evidence that the companions of host stars of planetary systems or…

地球与行星天体物理 · 物理学 2015-05-13 Richard J. Parker , Simon P. Goodwin

The Kozai mechanism for a hierarchical triple system could reduce the merger time of inner eccentric binary emitting gravitational waves (GWs), and has been qualitatively explained with the secular theory that is derived by averaging…

宇宙学与河外天体物理 · 物理学 2015-06-15 Naoki Seto

The presence of highly eccentric extrasolar planets in binary stellar systems suggests that the Kozai effect has played an important role in shaping their dynamical architectures. However, the formation of planets in inclined binary systems…

地球与行星天体物理 · 物理学 2015-05-28 Konstantin Batygin , Alessandro Morbidelli , Kleomenis Tsiganis

The Kozai mechanism often destabilises high inclination orbits. It couples changes in the eccentricity and inclination, and drives high inclination, circular orbits to low inclination, eccentric orbits. In a recent study of the dynamics of…

天体物理学 · 物理学 2009-11-13 P. E. Verrier , N. W. Evans

In recent years many binary minor planets (BMPs) have been discovered in the Solar system. Many models have been suggested for their formation, but these encounter difficulties explaining their observed characteristics. Here we show that…

天体物理学 · 物理学 2015-05-13 Hagai B. Perets , Smadar Naoz

Pairs of planets in a system may end up close to their host star on eccentric orbits as a consequence of planet planet scattering, Kozai or secular migration. In this scenario, general relativity and secular perturbations have comparable…

地球与行星天体物理 · 物理学 2020-02-12 Francesco Marzari , Makiko Nagasawa

We study the dynamical evolution of a test particle that orbits a star in the presence of an exterior massive planet, considering octupole-order secular interactions. In the standard Kozai mechanism (SKM), the planet's orbit is circular,…

地球与行星天体物理 · 物理学 2015-05-28 Yoram Lithwick , Smadar Naoz

Context. The presence of a stellar companion can strongly influence the architecture and long-term stability of planetary systems. Motivated by the discovery of exoplanets exhibiting extremely high eccentricities (e >= 0.8) in systems with…

地球与行星天体物理 · 物理学 2026-02-11 Milenne Ávila-Bravo , Carolina Charalambous , Claudia Aguilera-Gómez

We consider the dynamical evolution of bound, hierarchical triples of supermassive black holes that might be formed in the nuclei of galaxies undergoing sequential mergers. The tidal force of the outer black hole on the inner binary…

天体物理学 · 物理学 2009-11-07 Omer Blaes , Man Hoi Lee , Aristotle Socrates

We investigate the evolution of a multi--planet--disc system orbiting one component of a binary star system. The planet--disc system is initially coplanar but misaligned to the binary orbital plane. The planets are assumed to be giants that…

地球与行星天体物理 · 物理学 2020-01-08 Alessia Franchini , Rebecca G. Martin , Stephen H. Lubow

We investigate the Kozai mechanism in the context of near-Earth binaries and the Sun. The Kozai effect can lead to changes in eccentricity and inclination of the binary orbit, but it can be weakened or completely suppressed by other sources…

地球与行星天体物理 · 物理学 2015-06-03 Julia Fang , Jean-Luc Margot

This chapter concerns the long-term dynamical evolution of planetary systems from both theoretical and observational perspectives. We begin by discussing the planet-planet interactions that take place within our own Solar System. We then…

We study the dynamics of a planet on an orbit inclined with respect to a disc. If the initial inclination of the orbit is larger than some critical value, the gravitational force exerted by the disc on the planet leads to a Kozai cycle in…

地球与行星天体物理 · 物理学 2015-06-11 Jean Teyssandier , Caroline Terquem , John C. B. Papaloizou
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