Mass Derivation of planets K2-21b and K2-21c from Transit Timing Variations

While various indirect methods are used to detect exoplanets, one of the most effective and accurate methods is the transit method, which measures the brightness of a given star for periodic dips when an exoplanet is passing in front of the parent star. For systems with multiple transiting planets,...

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Veröffentlicht in:	arXiv.org 2023-05
Hauptverfasser:	Maryame El Moutamid, Stevenson, Kevin B, Quarles, Billy, Lewis, Nikole K, Erik Petigura Daniel Fabrycky, Bean, Jacob L, Dragomir, Diana, Kristin S Sotzenvand Michael W Werner
Format:	Artikel
Sprache:	eng
Schlagworte:	Dwarf stars Extrasolar planets Orbital resonances (celestial mechanics) Orbits Perturbation Physics - Earth and Planetary Astrophysics Planetary systems Stellar systems Transit Transit time
Online-Zugang:	Volltext
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