LATE ORBITAL INSTABILITIES IN THE OUTER PLANETS INDUCED BY INTERACTION WITH A SELF-GRAVITATING PLANETESIMAL DISK

By Harold Levison, A. Morbidelli, Kleomenis Tsiganis, D. Nesvorný, R. Gomes. 2011

228 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/fbe22d33af1008cc16ae65cb976d60e2794fa71f

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In Astronomy and Astrophysics

Citations in the corpus

Forming the cores of giant planets from the radial pebble flux in protoplanetary discs (2014, result): “To do so, a mass in planetesimals of about 50 ME is required (Morbidelli et al. 2007; Batygin & Brown 2010; Levison et al. 2011), in good agreement with our estimate.”
The timeline of the lunar bombardment: Revisited (2018, background): “Both solutions remain possible epending on the properties of the original trans-Neptunian disk Levison et al., 2011; Deienno et al., 2017 ).”
Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System (2012, background): “5 AU becomes 0 .44 yr−1. Francis (2005) determines the flux of new comets to be 2.”
Origin and Evolution of Short-period Comets (2017, background): “…studies, because of concerns with the delay of planetary instability, which was thought to be needed to explain the Late Heavy Bombardment (LHB) of the Moon and terrestrial planets (e.g., Gomes et al. 2005, Levison et al. 2011, Bottke et al. 2012, Marchi et al. 2012, Morbidelli et al. 2012).”
STATISTICAL STUDY OF THE EARLY SOLAR SYSTEM'S INSTABILITY WITH FOUR, FIVE, AND SIX GIANT PLANETS (2012, methodology): “Two potentially problematic issues of the original Nice model (hereafter ONM) were addressed by Morbidelli et al. (2007) and Levison et al. (2011).”
The primordial nucleus of comet 67P/Churyumov-Gerasimenko (2015, background): “They base this on Levison et al. (2011) who considered viscous stirring by 103 Pluto-sized bodies for 400 Myr.”
Water delivery and giant impacts in the 'Grand Tack' scenario (2014, unknown): “Their end locations coincide with the initial conditions in the Nice Model (e.g. Morbidelli et al., 2007; Levison et al., 2011), such that Jupiter (a = 5.”
YOUNG SOLAR SYSTEM's FIFTH GIANT PLANET? (2011, methodology): “This method was inspired by the recent study of the late instability that showed that planets can slowly exchange orbital energy with a distant planetesimal disk, and break from the resonances when the resonant amplitude exceeds certain limits (Levison et al. 2011).”
Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, background): “ons are appropriate for a giant planet instability at ~500 Myr (Nice model; late Morbidelli et al., 2007) that will place them and the outer ice giants (Neptune and 5 Uranus) on their current orbits (Levison et al., 2011). The treatment of the nebula gas and the giant planets are identical in each o”
EVIDENCE FOR A DISTANT GIANT PLANET IN THE SOLAR SYSTEM (2016, background): “…it is worth noting that although the primordial planetesimal disk of the solar system likely comprised tens of Earth masses (Tsiganis et al. 2005; Levison et al. 2008, 2011; Batygin et al. 2011), the vast majority of this material was ejected from the system by close encounters with the giant…”
CAPTURE OF TROJANS BY JUMPING JUPITER (2013, unknown): “Indeed, several inconsistencies of the ONM have been already pointed out leading to model’s revisions (Morbidelli et al. 2007, Levison et al. 2011).”
Populating the asteroid belt from two parent source regions due to the migration of giant planets—“The Grand Tack” (2012, background): “…mechanism is also at the heart of the Nice Model, whereby, after a long quiescent period in a close and compact configuration, the exchange of angular momentum between the massive primordial Kuiper Belt (30–50 Earth masses) and the planets breaks the planets out of resonance (Levison et al. 2011).”