O. Miloni
National University of La Plata
11 Papers
21 Citations
O. Miloni is an academic researcher from National University of La Plata. The author has contributed to research in topics: Equations of motion & Orbit. The author has an hindex of 4, co-authored 11 publications. Previous affiliations of O. Miloni include University of São Paulo.
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Papers
Tidal decay and orbital circularization in close-in two-planet systems
TL;DR: In this paper, the motion of two planets around a Sun-like star under the combined effects of mutual interaction and tidal dissipation is investigated using two different approaches: numerical simulation of the system evolution and stationary solutions of mean equations of motion.
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Angular momentum exchange during secular migration of two-planet systems
TL;DR: In this article, the authors investigate the evolution of two-planet coplanar systems evolving under mutual gravitational interactions and dissipative forces and show that each migration mechanism is characterized by a specific law of orbital angular momentum exchange.
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Analytical Proper Elements for the Hilda Asteroids I: Construction of a Formal Solution
TL;DR: In this article, the mathematical basis for the calculation of proper elements for asteroids in 3:2 mean-motion resonance with Jupiter from their osculating Keplerian elements is presented.
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•Journal Article
Distra: a code to find invisible exoplanets
TL;DR: In this article, the transit times of an exoplanet, which will differ from a Keplerian two-b ody series of transits if a second, non-transiting ex-planetary perturbation is perturbed, are compared.
Stability of Terrestrial Planets in the Habitable Zone of Gl 777 A, HD 72659, Gl 614, 47 Uma and HD 4208
N. Asghari,C. Broeg,L. Carone,Rigoberto A. Casas-Miranda,J. C. Castro Palacio,I. Csillik,Rudolf Dvorak,F. Freistetter,G. Hadjivantsides,Hauke Hussmann,A. Khramova,M. Khristoforova,I. Khromova,I. Kitiashivilli,S. Kozlowski,T. Laakso,T. Laczkowski,D. Lytvinenko,O. Miloni,Ryuji Morishima,Amaya Moro-Martin,V. Paksyutov,A. Pal,Vinod Patidar,B. Pecnik,O. Peles,J. Pyo,Thomas R. Quinn,Adrián Rodríguez,C. Romano,Eeshankur Saikia,Joachim Stadel,Marco Thiel,N. Todorovic,Dimitri Veras,E. Vieira Neto,Jozef Vilagi,W. von Bloh,R. Zechner,E. Zhuchkova +39 more
TL;DR: In this article, the authors investigated the mean motion resonances between fictitious terrestrial planets and the existing gas giants in these five extrasolar systems, and then a fine grid of initial conditions for a potential terrestrial planet within the HZ was chosen for each system, from which the stability of orbits was then assessed by direct integrations over a time interval of 1 million years.