Origin of the orbital architecture of the giant planets of the Solar System

By Kleomenis Tsiganis, Rodney Gomes, A. Morbidelli, Harold Levison. Nature, 2005

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View Paper: https://www.semanticscholar.org/paper/02640f28ab5c2fe5a883c855fd0bc77505b48a00

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In Astronomy and Astrophysics

Citations in the corpus

YOUNG SOLAR SYSTEM's FIFTH GIANT PLANET? (2011, background): “In the later case, the instability is produced when Jupiter and Saturn cross a major mean motion resonance (Tsiganis et al. 2005; also known as the Nice model).”
Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, methodology): “formation, the “Nice model” (Tsiganis et al. 2005; Morbidelli et al. 2007) has been modified”
EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER's ORBIT (2010, methodology): “…distance travelled by Jupiter and Saturn would result in practically the same dynamics because of two reasons: First, the asteroid belt is only affected by secular resonances whenPS/PJ > 2 (Gomes, 1997) i.e. towards the end of migration (Malhotra, 1993; Tsiganis et al., 2005; Gomes et al., 2005).”
Terrestrial planet formation with strong dynamical friction (2006, background): “It is thus possible that, in the Nice Model, Jupiter and Saturn could begin with eccentricities intermediate between 0 and their current values, although there is currently no well-defined model of how this could occur, and would decay to ∼0 well before the 2:1 resonance crossing 700 Myr later.”
Chemical enrichment of giant planets and discs due to pebble drift (2017, background): “Models can place constraints on their location during terrestrial planet formation, requiring them to be near their current locations during the process (e.g. Tsiganis et al. 2005; Raymond et al. 2006; Walsh et al. 2011; Agnor & Lin 2012; Raymond et al. 2014).”
NEAR-INFRARED SPECTROSCOPY OF TROJAN ASTEROIDS: EVIDENCE FOR TWO COMPOSITIONAL GROUPS (2008, background): “Tsiganis et al. (2005) have suggested that during this early migration, Jupiter and Saturn crossed their 2:1 mean motion resonance, which in turn initially destabilized the orbits of Uranus and Neptune, wreaking a fair bit of havoc across the Solar System.”
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, background): “The subsequent dynamical history of the solar system may have shifted their positions and greatly reduced their numbers (e.g., Gomes et al. 2005, Morbidelli et al. 2005, Tsiganis et al. 2005, Minton and Malhotra 2009).”
JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system (2013, background): “The study of the impact craters, their sizes and distribution provides important information about the age of the surfaces of the satellites and helps to comprehend the evolution of the early Solar System, in particular the reality and the characteristics of the Late Heavy Bombardment that has been ”
The dynamics of Jupiter and Saturn in the gaseous protoplanetary disk (2007, background): “…to the LHB, this model explains the current orbital architecture of the giant planets (orbital separations, eccentricities and mutual inclinations; Tsiganis et al., 2005) the origin and orbital distribution of the Trojans of Jupiter (Morbidelli et al., 2005) and the structure of the Kuiper belt…”
COMETARY ORIGIN OF THE ZODIACAL CLOUD AND CARBONACEOUS MICROMETEORITES. IMPLICATIONS FOR HOT DEBRIS DISKS (2009, background): “The Nice model is compelling because it can explain many of the characteristics of the outer solar system, (Tsiganis et al., 2005; Morbidelli et al., 2005; Nesvorný et al., 2007; Levison et al., 2008; Nesvorný and Vokrouhlický, 2009).”
Building the terrestrial planets: Constrained accretion in the inner Solar System (2009, methodology): “The CJS, JSRES and JSRESECC simulations all follow from the Nice model and assume that Jupiter and Saturn’s orbits changed significantly after their formation, with Saturn migrating outward and Jupiter inward (Tsiganis et al., 2005).”
Atmospheric Escape and Evolution of Terrestrial Planets and Satellites (2008, background): “However, a new dynamical model for Solar System formation (Tsiganis et al. 2005; Gomes et al. 2005) suggests that the “pulse” hypothesis may indeed have been correct.”
STATISTICAL STUDY OF THE EARLY SOLAR SYSTEM'S INSTABILITY WITH FOUR, FIVE, AND SIX GIANT PLANETS (2012, background): “Morbidelli et al. (2007) studied the dynamical instability starting from the resonant planetary systems and showed that the orbit evolution of planets was similar to that of the ONM.”
Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune (2007, methodology): “, 2005) and of Neptune (Tsiganis et al., 2005; Sheppard and Trujillo, 2006), and the origin of at least some of the giant planet irregular satellites (Nesvorný et al.”