Modern celestial mechanics : aspects of solar system dynamics
By A. Morbidelli. 2002
442 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/05a1b074f5d84e53f88497adeac003e94cd7427f
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- D. Nesvorný
- A. Morbidelli
- William Bottke
- K. Batygin
- Harold Levison
- David Vokrouhlický
- R. Brasser
- Fred C. Adams
Citations in the corpus
- Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture (2007, result): “Our investigation extends the previous works by Masset and Snellgrove (2001) and Morbidelli and Crida (2007, MC07), which focussed on the dynamics of the Jupiter-Saturn system.”
- DISSIPATIVE DIVERGENCE OF RESONANT ORBITS (2012, background): “This is a well-known fact for first order resonances (see for example Ch.9 of Morbidelli (2002))1.”
- Scenarios for the Origin of the Orbits of the Trans-Neptunian Objects 2000 CR105 and 2003 VB12 (Sedna) (2004, methodology): “…planets (assumed to be on coplanar and circular orbits) and a massive disk situated on the planets’ orbital plane can be analytically computed with a trivial adaptation of the approach usually followed to compute the effects of the Kozai resonance (see Thomas & Morbidelli 1996; Morbidelli 2002).”
- The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? (2002, methodology): “The proper elements are analytically defined as constants of motion of a suitably simplified dynamical system, achieved from the original dynamical system using the classical tools of the “normal form” theory (Milani and Kneˇ zevi´ c 1990; see also chapter 8 of Morbidelli 2002 ).”
- The Eccentric Kozai-Lidov Effect and Its Applications (2016, background): “This approximation has an analytical solution which describes (for initially highly inclined orbits ∼ 40◦−140◦, see below) the large amplitude oscillations between the inner orbit’s eccentricity and inclination with respect to the outer orbit (e.g., Kinoshita and Nakai 1999; Morbidelli 2002).”
- IN SITU FORMATION AND DYNAMICAL EVOLUTION OF HOT JUPITER SYSTEMS (2015, background): “We note that orbital excitation by sweeping secular resonances has previously been studied within the context of the solar system (see e.g. Ward et al. 1976; Ward 1981; Nagasawa and Ida 2000; Nagasawa et al. 2002; Minton and Malhotra 2011; Agnor and Lin 2012).”
- Sub-arcsec imaging of the AB Aur molecular disk and envelope at millimeter wavelengths: a non Keplerian disk (2005, background): “Monnier & Millan-Gabet (2002) have shown that in such objects, the very inner dust disk is truncated by sublimation of the dust at temperature around∼ 1500 K.”
- The planet nine hypothesis (2019, methodology): “More specifically, while MMRs may modulate the long-term stability of KBOs through the phase-locking mechanism (Morbidelli, 2002), the clustering of orbits in physical space, as well as excitation of extreme inclinations of long-period TNOs is largely a secular effect.”
- EVIDENCE FOR A DISTANT GIANT PLANET IN THE SOLAR SYSTEM (2016, background): “Viewed in this context, the origins of such bodies stem directly from the conventional scattered disk, and should on average exhibit the same physical characteristics as other large members of the Kuiper belt.”
- Origin and Evolution of Near-Earth Objects (2002, background): “The latter can be identified with the mean precession frequency of Saturn’s longitude of perihelion, but it is also relevant in the secular oscillation of the eccentricity of Jupiter (see chapter 7 of Morbidelli, 2002 ).”
- One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c (2015, methodology): “For more details on the NITES telescope we refer the reader to McCormac et al. (2014). One transit of K2-19b was observed on 2015 Feb.”
- Constructing the secular architecture of the solar system II: The terrestrial planets (2009, unknown): “9 Gyr ago was relatively cool (i.e. the impact rate was low; Mojzsis et al. 2001), and that strong heating events, probably associated with impacts, happened approximately 3.”
- EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER's ORBIT (2010, background): “In fact, it is well know that mean motion resonances are stable if Jupiter follows a circular orbit (Morbidelli, 2002).”