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Thousands of confirmed and candidate exoplanets have been identified in recent years. Consequently, theoretical research on the formation and dynamical evolution of planetary systems has seen a boost, and the processes of planet-planet…

地球与行星天体物理 · 物理学 2016-09-06 M. B. N. Kouwenhoven , Qi Shu , Maxwell Xu Cai , Rainer Spurzem

Among the hundred or so extrasolar planets discovered to date, 19 are orbiting a component of a double or multiple star system. In this paper, we discuss the properties of these planets and compare them to the characteristics of planets…

天体物理学 · 物理学 2009-11-10 A. Eggenberger , S. Udry , M. Mayor

Instabilities and strong dynamical interactions between multiple giant planets have been proposed as a possible explanation for the surprising orbital properties of extrasolar planetary systems. In particular, dynamical instabilities seem…

天体物理学 · 物理学 2007-05-23 Eric B. Ford , Frederic A. Rasio , Kenneth Yu

With the increasing number of detected exoplanet samples, the statistical properties of planetary systems have become much clearer. In this review, we summarize the major statistics that have been revealed mainly by radial velocity and…

地球与行星天体物理 · 物理学 2015-06-05 J. -L. Zhou , J. -W. Xie , H. -G. Liu , H. Zhang , Y. -S. Sun

(Abridged) In planetary systems with two or more giant planets, dynamical instabilities can lead to collisions or ejections through strong planet--planet scattering. Previous studies for simple initial configurations with two equal-mass…

天体物理学 · 物理学 2008-12-18 Eric B. Ford , Frederic A. Rasio

The known extrasolar multiple-planet systems share a surprising dynamical attribute: they cluster just beyond the Hill stability boundary. Here we show that the planet-planet scattering model, which naturally explains the observed exoplanet…

地球与行星天体物理 · 物理学 2011-02-11 Sean N. Raymond , Rory Barnes , Dimitri Veras , Philip J. Armitage , Noel Gorelick , Richard Greenberg

We study the final architecture of planetary systems that evolve under the combined effects of planet-planet and planetesimal scattering. Using N-body simulations we investigate the dynamics of marginally unstable systems of gas and ice…

地球与行星天体物理 · 物理学 2009-07-22 Sean N. Raymond , Philip J. Armitage , Noel Gorelick

The basic geometry of the Solar System -- the shapes, spacings, and orientations of the planetary orbits -- has long been a subject of fascination as well as inspiration for planet formation theories. For exoplanetary systems, those same…

地球与行星天体物理 · 物理学 2015-10-19 Joshua N. Winn , Daniel C. Fabrycky

Doppler spectroscopy has detected 136 planets around nearby stars. A major puzzle is why their orbits are highly eccentric, while all planets in our Solar System are on nearly circular orbits, as expected if they formed by accretion…

天体物理学 · 物理学 2007-05-23 Eric B. Ford , Verene Lystad , Frederic A. Rasio

Just fourteen years ago the Solar System represented the only known planetary system in the Galaxy, and conceptions of planet formation were shaped by this sample of one. Since then, 320 planets have been discovered orbiting 276 individual…

地球与行星天体物理 · 物理学 2015-05-13 John A. Johnson

Doppler planet searches revealed that many giant planets orbit close to their host star or in highly eccentric orbits. These and subsequent observations inspired new theories of planet formation that invoke gravitation interactions in…

地球与行星天体物理 · 物理学 2015-06-19 Eric B. Ford

In most extrasolar planetary systems, the present orbits of known giant planets admit the existence of stable terrestrial planets. Those same giant planets, however, have typically eccentric orbits that hint at violent early dynamics less…

天体物理学 · 物理学 2009-11-10 Dimitri Veras , Philip J. Armitage

The Solar System hosts the most studied and best understood major and minor planetary bodies - and the only extraterrestrial bodies to have been visited by spacecraft. The Solar System therefore provides important constraints on both the…

地球与行星天体物理 · 物理学 2025-08-04 Anders Johansen , Michele T. Bannister , Luke Dones , Seth Jacobson , Kelsi Singer , Kathryn Volk , Maria Womack

The apparent regularity of the motion of the giant planets of our solar system suggested for decades that said planets formed onto orbits similar to the current ones and that nothing dramatic ever happened during their lifetime. The…

地球与行星天体物理 · 物理学 2020-07-17 Alessandro Morbidelli

Recent observations have revealed two new classes of planetary orbits. Rossiter- Mclaughlin (RM) measurements have revealed hot Jupiters in high-obliquity orbits. In addition, direct-imaging has discovered giant planets at large (~ 100 AU)…

地球与行星天体物理 · 物理学 2015-05-20 Sourav Chatterjee , Eric B. Ford , Frederic A. Rasio

The large eccentricities of many giant extrasolar planets may represent the endpoint of gravitational scattering in initially more crowded systems. If so, the early evolution of the giant planets is likely to be more restrictive of…

天体物理学 · 物理学 2009-11-11 Dimitri Veras , Philip J. Armitage

Transiting circumbinary planets discovered by Kepler provide unique insight into binary star and planet formation. Several features of this new found population, for example the apparent pile-up of planets near the innermost stable orbit,…

地球与行星天体物理 · 物理学 2016-06-15 Rachel A. Smullen , Kaitlin M. Kratter , Andrew Shannon

Over the past several decades, thousands of planets have been discovered outside of our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the…

Extrasolar multiple-planet systems provide valuable opportunities for testing theories of planet formation and evolution. The architectures of the known multiple-planet systems demonstrate a fascinating level of diversity, which motivates…

地球与行星天体物理 · 物理学 2009-11-13 Robert A. Wittenmyer , Michael Endl , William D. Cochran , Harold F. Levison , Gregory W. Henry

Evidence of mutually inclined planetary orbits has been reported for giant planets these last years. Here we aim to study the impact of eccentric and inclined massive giant planets on the terrestrial planet formation process, and…

地球与行星天体物理 · 物理学 2018-06-06 Sotiris Sotiriadis , Anne-Sophie Libert , Sean N. Raymond
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