Article, 2024

Revealing the dynamical properties of Jupiter-size exoplanets on elliptic orbits

CHAOS SOLITONS & FRACTALS, ISSN 0960-0779, Volume 184, 10.1016/j.chaos.2024.114969

Contributors

Zotos, Euaggelos E. (Corresponding author) [1] [2] Moneer, Eman M. [3] Dubeibe, Fredy L. [4] Hinse, Tobias C. [5]

Affiliations

  1. [1] Aristotle Univ Thessaloniki, Sch Sci, Dept Phys, GR-54124 Thessaloniki, Greece
    2. [NORA names: Greece; Europe, EU; OECD];
  2. [2] RUDN Univ, Peoples Friendship Univ Russia, SM Nikolskii Math Inst, Moscow 117198, Russia
    3. [NORA names: Russia; Europe, Non-EU];
  3. [3] Princess Nourah Bint Abdulrahman Univ, Coll Sci, Dept Phys, POB 84428, Riyadh 11671, Saudi Arabia
    4. [NORA names: Saudi Arabia; Asia, Middle East];
  4. [4] Univ Llanos, Fac Ciencias Humanas & Educ, Villavicencio 500003, Colombia
    5. [NORA names: Colombia; America, South; OECD];
  5. [5] Univ Southern Denmark, Dept Phys Chem & Pharm, Campusvej 55, DK-5230 Odense M, Denmark
    6. [NORA names: SDU University of Southern Denmark; University; Denmark; Europe, EU; Nordic; OECD]

Abstract

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Keywords

Dynamical evolution and stability -, General - planets and satellites, Numerical, Planets and satellites, planet-star interactions - methods

Data Provider: Clarivate

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