Dynamical origin of Dimorphos from fast spinning Didymos
Didymos is a binary near-Earth asteroid. It is the target of the DART and HERA space
missions. The primary body, Didymos, rotates close to the spin at which it is expected to …
missions. The primary body, Didymos, rotates close to the spin at which it is expected to …
Dynamics around non-spherical symmetric bodies: II. The case of a prolate body
Dynamic exploration around non-spherical bodies has increased in recent decades due to
the interest in studying the motion of spacecraft orbits, moons, and particle ring around these …
the interest in studying the motion of spacecraft orbits, moons, and particle ring around these …
Revisiting Dimorphos formation: A pyramidal regime perspective and application to Dinkinesh's satellite
Dimorphos' oblate shape challenges formation models. Landslides on Didymos, induced by
YORP effect, probably created a debris ring from which Dimorphos would have formed …
YORP effect, probably created a debris ring from which Dimorphos would have formed …
The stability around Chariklo and the confinement of its rings
Context. Chariklo has two narrow and dense rings, C1R and C2R, located at 391 km and
405 km, respectively. Aims. In the light of new stellar occultation data, we study the stability …
405 km, respectively. Aims. In the light of new stellar occultation data, we study the stability …
Exploring the recycling model of Phobos formation: rubble-pile satellites
Phobos is the target of the return sample mission Martian Moons eXploration by JAXA that
will analyze in great detail the physical and compositional properties of the satellite from …
will analyze in great detail the physical and compositional properties of the satellite from …
Dynamics around non-spherical symmetric bodies–I. The case of a spherical body with mass anomaly
The space missions designed to visit small bodies of the Solar system boosted the study of
the dynamics around non-spherical bodies. In this vein, we study the dynamics around a …
the dynamics around non-spherical bodies. In this vein, we study the dynamics around a …
A comparison of centring algorithms in the astrometry of Cassini imaging science subsystem images and Anthe's astrometric reduction
QF Zhang, XM Zhou, Y Tan, V Lainey… - Monthly Notices of …, 2021 - academic.oup.com
In the caviar software package, a standard tool for astrometry of images from the Cassini
imaging science subsystem (ISS), Gaussian fitting is used to measure the centre of point-like …
imaging science subsystem (ISS), Gaussian fitting is used to measure the centre of point-like …
Dynamical stability in the vicinity of Saturnian small moons: the cases of Aegaeon, Methone, Anthe, and Pallene
A Rodríguez, N Callegari Jr - Monthly Notices of the Royal …, 2021 - academic.oup.com
In this work we analyse the orbital evolution and dynamical stability in the vicinity of the
small Saturnian moons Aegaeon, Methone, Anthe, and Pallene. We numerically resolve the …
small Saturnian moons Aegaeon, Methone, Anthe, and Pallene. We numerically resolve the …
Numerical analysis of processes for the formation of moonlets confining the arcs of Neptune
G Madeira, SM Giuliatti Winter - Monthly Notices of the Royal …, 2022 - academic.oup.com
ABSTRACT The arcs of Neptune–Fraternité, Egalité, Liberté, and Courage–are four
incomplete rings immersed in the Adams ring. A recent confinement model for the arcs …
incomplete rings immersed in the Adams ring. A recent confinement model for the arcs …
Long-term dynamical evolution of Pallene (Saturn XXXIII) and its diffuse, dusty ring
MA Muñoz-Gutiérrez… - Monthly Notices of …, 2022 - academic.oup.com
The distinctive set of Saturnian small satellites, Aegaeon, Methone, Anthe, and Pallene,
constitutes an excellent laboratory to understand the evolution of systems immersed in co …
constitutes an excellent laboratory to understand the evolution of systems immersed in co …