From the 1 of 4 linked papers with an AI index.
4 papers
Tidal evolution of packed moon systems around an Earth-mass planet
Alan Briseño, Billy Quarles, Marialis Rosario-Franco
The paper uses N-body and tidal simulations to determine how many tightly packed moons of various masses can stably orbit an Earth‑mass planet, finding limits that depend on tidal…
Tidally Torn: Why the Most Common Stars May Lack Large, Habitable-Zone Moons
Shaan D. Patel, Billy Quarles, Nevin N. Weinberg +1
Earth-like planets in the habitable zone (HZ) of M-dwarfs have recently been targeted in the search for exomoons. We study the stability and lifetime of large (Luna-like) moons, ac…
Can Moons Exist around the Habitable-zone Planet K2-18b?
Shaan D. Patel, Billy Quarles, Manfred Cuntz +1
K2-18b closely orbits a nearby M3 dwarf within its habitable zone, where this planet could be either a super-Earth or a mini-Neptune. Recent studies using transit spectroscopy sugg…
Orbital Stability of Hierarchical 3 and 4-Body Systems with Inclination: Results for Kepler-1625, 1708, and HD 23079
Shaan D. Patel, Billy Quarles, Manfred Cuntz
As the number of potential exomoon candidates grows, there is a heightened motivation of pursing orbital stability analyses. In this work, we provide an in-depth investigation into…