Capture of Irregular Satellites during Planetary Encounters

By D. Nesvorný, David Vokrouhlický, A. Morbidelli. 2007

216 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/385d61fa748249b801f2d2cea1c258af964a7061

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In Astronomy and Astrophysics

Citations in the corpus

CAPTURE OF TROJANS BY JUMPING JUPITER (2013, background): “This is encouraging because it favorably compares with estimates obtained by other means (e.g., Nesvorný et al. 2007, Levison et al. 2008, Charnoz et al. 2009, Morbidelli et al. 2009a).”
EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER's ORBIT (2010, background): “Capture of the Irregular satellites of Jupiter Nesvorný et al. (2007) showed that the capture of irregularsatellites is a generic outcome of planet-planet encounters and reproduces their orbital distribution well.”
The timeline of the lunar bombardment: Revisited (2018, background): “ planet instability could have produced the putative cataclysm. While the evidence for a giant planet instability strengthened over the years with the detailed analysis of the Solar System structure (Nesvorny et al., 2007; Nesvorny and Morbidelli, 2012; Brasser and Morbidelli, 2013; Nesvorny et al. ”
STATISTICAL STUDY OF THE EARLY SOLAR SYSTEM'S INSTABILITY WITH FOUR, FIVE, AND SIX GIANT PLANETS (2012, background): “…model is compelling because it explains the separations, eccentricities, and inclinations of the outer planets (Tsiganis et al. 2005), and many properties of the populations of small bodies (Morbidelli et al. 2005, Nesvorný et al. 2007, Levison et al. 2008, 2009, Nesvorný & Vokrouhlický 2009).”
Mercury’s Weather-Beaten Surface: Understanding Mercury in the Context of Lunar and Asteroidal Space Weathering Studies (2014, methodology): “From dynamical models of solar system evolution modeling derived from the socalled “Nice model” (Morbidelli et al. 2005; Nesvorny et al. 2007; Charnoz et al. 2009; Broz et al. 2011), including the concept of an extended or “E-belt” of early asteroids (Bottke et al. 2012), in conjunction with the…”
YOUNG SOLAR SYSTEM's FIFTH GIANT PLANET? (2011, background): “To explain the observed populations of the irregular moons that are roughly similar at each planet (Jewitt & Haghighipour 2007), all planets –including Jupiter– must participate in encounters (Nesvorný et al. 2007).”
Origin and Evolution of Short-period Comets (2017, background): “…asteroid belt (Levison et al. 2009, Vokrouhlický et al. 2016), Jupiter Trojans (Morbidelli et al. 2005, Nesvorný et al. 2013), irregular satellites (Nesvorný et al. 2007, 2014), Kuiper belt (Malhotra 1993, Gomes 2003, Hahn & Malhotra 2005; Levison et al. 2008; Dawson & Murray-Clay 2012;…”
Constructing the secular architecture of the solar system II: The terrestrial planets (2009, unknown): “For instance, this happened in one simulation out of six in Gomes et al. (2005), and in two simulations out of 14 in Nesvorný et al. (2007).”
LATE ORBITAL INSTABILITIES IN THE OUTER PLANETS INDUCED BY INTERACTION WITH A SELF-GRAVITATING PLANETESIMAL DISK (2011, background): “It reproduces the number and the inclination distribution of irregular satellites of the giant planets (Nesvorný et al. 2007; Bottke et al. 2010).”
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).”
Populating the asteroid belt from two parent source regions due to the migration of giant planets—“The Grand Tack” (2012, background): “The essential characteristics of the Nice Model are quite different from the Grand Tack, as the migration of the giant planets during the Grand Tack is caused by interactions with the gas-disk, while migration during the Nice Model is driven by the gravitational scattering of planetesimals from a ma”