Celestial Mechanics and Dynamical Astronomy, v. 94, n. 1, p. 83-104, 2006. http://dx.doi.org/10.1007/s10569-005-1472-2International audienc
The Lagrange’s planetary equations written in terms of the classical orbital elements have the disad...
Context. In June 2021, the discovery of an unusual comet C/2014 UN271 (Bernardinelli-Bernstein) was ...
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
The aim of this work is to investigate the main dominant terms of lunisolar perturbations that affec...
Long period perturbations in motion of small eccentricity satellites and analysis of Alouette I and ...
The two dominant features in the distribution of orbital parameters for close-in exo-planets are the...
A particular case of steady state and spherical symmetry - the so-called logarithmic potential intro...
The semi-analytical model (based on the averaging technique) for long-term orbital evolution has pro...
Eccentric orbits in the third-body perturbed problem are evaluated in the context of planetary moon ...
Planets on initially circular orbits are typically more dynamically stable than planets initially ha...
The influence of non-gravitational effects on the motion of long-period comets is analyzed. Investig...
Janus and Epimetheus are famously known for their dis-tinctive horseshoe-shaped orbits resulting fro...
Radial velocity surveys are beginning to reach the time baselines required to detect Jupiter analogs...
This paper investigates the long-term evolution of spacecraft in Highly Elliptical Orbits (HEOs). Th...
The lunar and solar gravitational perturbations coupled with the J 2 effect acting on Earth-orbiting...
The Lagrange’s planetary equations written in terms of the classical orbital elements have the disad...
Context. In June 2021, the discovery of an unusual comet C/2014 UN271 (Bernardinelli-Bernstein) was ...
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
The aim of this work is to investigate the main dominant terms of lunisolar perturbations that affec...
Long period perturbations in motion of small eccentricity satellites and analysis of Alouette I and ...
The two dominant features in the distribution of orbital parameters for close-in exo-planets are the...
A particular case of steady state and spherical symmetry - the so-called logarithmic potential intro...
The semi-analytical model (based on the averaging technique) for long-term orbital evolution has pro...
Eccentric orbits in the third-body perturbed problem are evaluated in the context of planetary moon ...
Planets on initially circular orbits are typically more dynamically stable than planets initially ha...
The influence of non-gravitational effects on the motion of long-period comets is analyzed. Investig...
Janus and Epimetheus are famously known for their dis-tinctive horseshoe-shaped orbits resulting fro...
Radial velocity surveys are beginning to reach the time baselines required to detect Jupiter analogs...
This paper investigates the long-term evolution of spacecraft in Highly Elliptical Orbits (HEOs). Th...
The lunar and solar gravitational perturbations coupled with the J 2 effect acting on Earth-orbiting...
The Lagrange’s planetary equations written in terms of the classical orbital elements have the disad...
Context. In June 2021, the discovery of an unusual comet C/2014 UN271 (Bernardinelli-Bernstein) was ...
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
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