2021/01/31 by Yuan-Zhe Dai, Hui-Gen Liu, Dong-Sheng An +1
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Hot Jupiter #Kepler #Planet #Planetary habitability #Planetary system #Stars #Stellar, planetary, and galactic studies #Terrestrial planet #astro-ph.EP #astro-ph.GA #astro-ph.SR
paper · pdf · doi:10.3847/1538-3881/ac00ad
published as AJ, 162, 46 (2021) · 30 pages, 17 figures, accepted for publication in AJ
openalex created_date 2021/02/01 · openalex publication_date 2021/07/07 · arxiv created 2021/07/12 · arxiv updated 2021/07/13 · openalex updated_date 2026/08/05
Abstract The dynamical history of stars influences the formation and evolution of planets significantly. To explore the influence of dynamical history on the planet formation and evolution using observations, we assume stars that experienced significantly different dynamical histories tend to have different relative velocities. Utilizing the accurate Gaia–Kepler Stellar Properties Catalog, we select single main-sequence stars and divide these stars into three groups according to their relative velocities, i.e., high- V , medium- V , and low- V stars. After considering the known biases from Kepler data and adopting prior and posterior correction to minimize the influence of stellar properties on planet occurrence rate, we find that high- V stars have a lower occurrence rate of super-Earths and sub-Neptunes (1–4 R ⊕ , P < 100 days) and a higher occurrence rate of sub-Earth (0.5–1 R ⊕ , P < 30 days) than low- V stars. Additionally, high- V stars have a lower occurrence rate of hot Jupiter-sized planets (4–20 R ⊕ , P < 10 days) and a slightly higher occurrence rate of warm or cold Jupiter-sized planets (4–20 R ⊕ , 10 < P < 400 days). After investigating multiplicity and eccentricity, we find that high- V planet hosts prefer a higher fraction of multiplanet systems and lower average eccentricity, which are consistent with the eccentricity–multiplicity dichotomy of Kepler planetary systems. All of these statistical results favor the scenario that high- V stars with large relative velocity may experience fewer gravitational events, while low- V stars may be influenced by stellar clustering significantly.