Secular Resonances: New Results

1988 ◽  
pp. 113-117
Author(s):  
Ch. Froeschlé ◽  
H. Scholl
Keyword(s):  
Secular Resonances

scholarly journals Asteroid Proper Elements: The Big Picture

1994 ◽  
Vol 160 ◽  
pp. 143-158 ◽  
Author(s):  
Zoran Knežević ◽  
Andrea Milani
Keyword(s):  
Point Of View ◽  
Dynamical Structure ◽  
Main Belt ◽  
Secular Resonances ◽  
Mean Motion Resonances ◽  
Mean Motion ◽  
Proper Elements ◽  
Big Picture ◽  
Linear And Nonlinear ◽  
Asteroid Families

Four perturbation theories presently used to compute asteroid proper elements are reviewed, and their results are briefly discussed (Milani and Knežević, 1990, 1992, 1994, for low to moderate eccentricity/inclination main belt objects; Lemaitre and Morbidelli, 1994, for high e, I objects; Milani, 1993, for Trojans; Schubart, 1982, 1991 for Hildas). The most important recent improvements are described, in particular those pertaining to the upgrades of the previous analytic and semianalytic solutions. The dynamical structure of the asteroid main belt, as defined by the low order mean motion resonances and by linear and nonlinear secular resonances, is considered from the point of view of the effects of these resonances on the accuracy and/or reliability of the computation of proper elements and on the reliability of the identification of asteroid families.

Trojan Orbits in Secular Resonances

1984 ◽  
pp. 425-434
Author(s):  
R. Bien ◽  
J. Schubart
Keyword(s):  
Secular Resonances

scholarly journals Positions of the secular resonances in the primordial Kuiper Belt disk

Icarus ◽  
2019 ◽  
Vol 334 ◽  
pp. 99-109 ◽  
Author(s):  
D. Baguet ◽  
A. Morbidelli ◽  
J.-M. Petit
Keyword(s):  
Kuiper Belt ◽  
Secular Resonances

Secular Resonances in Mean Motion Commensurabilities: The 4/1, 3/1, 5/2, and 7/3 Cases

Icarus ◽  
1995 ◽  
Vol 114 (1) ◽  
pp. 33-50 ◽  
Author(s):  
Michèle Moons ◽  
Alessandro Morbidelli
Keyword(s):  
Secular Resonances ◽  
Mean Motion

scholarly journals The Distribution of Asteroidal Dust in the Inner Solar System

2004 ◽  
Vol 202 ◽  
pp. 184-186
Author(s):  
Keith Grogan ◽  
S.F. Dermott ◽  
T.J.J. Kehoe
Keyword(s):  
Solar System ◽  
Parent Body ◽  
Asteroid Belt ◽  
Dust Particles ◽  
Secular Resonances ◽  
Level Of Confidence ◽  
Asteroidal Dust

In this paper we demonstrate how the action of secular resonances near the inner edge of the asteroid belt strongly effects the inclinations and eccentricities of asteroidal dust particles, such that they lose the orbital characteristics of their parent body and are dispersed into the zodiacal background. As a consequence, it may not be possible to relate the distribution of interplanetary material at 1 AU to given asteroidal or cometary sources with the level of confidence previously imagined.

scholarly journals White dwarf pollution by asteroids from secular resonances

2018 ◽  
Vol 480 (1) ◽  
pp. 57-67 ◽  
Author(s):  
Jeremy L Smallwood ◽  
Rebecca G Martin ◽  
Mario Livio ◽  
Stephen H Lubow
Keyword(s):  
White Dwarf ◽  
Secular Resonances

The Solar Nebula, Secular Resonances, Gas Drag, and the Asteroid Belt

Icarus ◽  
1997 ◽  
Vol 129 (1) ◽  
pp. 134-146 ◽  
Author(s):  
Myron Lecar ◽  
Fred Franklin
Keyword(s):  
Solar Nebula ◽  
Asteroid Belt ◽  
Secular Resonances ◽  
Gas Drag

Possible effects of secular resonances in Phobos and Triton

2002 ◽  
Vol 50 (1) ◽  
pp. 63-77 ◽  
Author(s):  
Tadashi Yokoyama
Keyword(s):  
Secular Resonances
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