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Modelling the secular evolution of migrating planet pairs
(WILEY-BLACKWELL, 2011)
The subject of this paper is the secular behaviour of a pair of planets evolving under dissipative forces. In particular, we investigate the case when dissipative forces affect the planetary semimajor axes and the planets ...
On the location of the ring around the dwarf planet Haumea
(2019-04-11)
The recently discovered ring around the dwarf planet (136108) Haumea is located near the 1:3 resonance between the orbital motion of the ring particles and the spin of Haumea. In the current work, we study the dynamics of ...
APOPHIS - effects of the 2029 Earth's encounter on the surface and nearby dynamics (vol 510, pg 95, 2022)
(Oxford Univ Press, 2022-02-24)
Coupled orbital and spin evolution of the CoRoT-7 two-planet system using a Maxwell viscoelastic rheology
(2016-01-01)
We investigate the orbital and rotational evolution of the CoRoT-7 two-planet system, assuming that the innermost planet behaves like a Maxwell body. We numerically resolve the coupled differential equations governing the ...
Role of gaseous giants in the dynamical evolution of terrestrial planets and water delivery in the habitable zone
(Oxford University Press, 2018-11)
In this research, we study the effects of a single giant planet on the dynamical evolution of water-rich embryos and planetesimals, located beyond the snow line of systems around Sun-like stars, in order to determine what ...
Constraining the nature of the possible extrasolar PDS110b ring system
(2021-08-01)
The young star PDS110 in the Ori OB1a association underwent two similar eclipses in 2008 and 2011, each of which lasted for a period of at least 25 days. One plausible explanation for these events is that the star was ...