# KELT-22Ab: A Massive, Short-Period Hot Jupiter Transiting a Near-solar Twin

@article{LabadieBartz2019KELT22AbAM,
title={KELT-22Ab: A Massive, Short-Period Hot Jupiter Transiting a Near-solar Twin},
author={J. Labadie-Bartz and J. Rodriguez and K. Stassun and D. Ciardi and M. Johnson and B. S. Gaudi and K. Penev and A. Bieryla and D. Latham and J. Pepper and K. Collins and P. Evans and H. Relles and R. Siverd and J. Bento and Xinyu Yao and C. Stockdale and T. Tan and G. Zhou and K. Col'on and J. Eastman and M. Albrow and A. Malpas and D. Bayliss and T. Beatty and V. Bozza and D. Cohen and I. Curtis and D. Depoy and D. Feliz and B. Fulton and J. Greg{\'o}rio and D. James and H. Jang-Condell and E. Jensen and J. Johnson and S. Johnson and M. Joner and J. Kielkopf and R. Kuhn and M. Lund and Mark Manner and J. Marshall and N. McCrady and Kim K. McLeod and T. Oberst and M. Penny and Rick Pogge and P. Reed and D. Sliski and D. Stephens and D. J. Stevens and M. Trueblood and P. Trueblood and S. Villanueva and R. Wittenmyer and J. Wright and R. Zambelli and P. Berlind and M. Calkins and G. Esquerdo},
journal={Astrophysical Journal Supplement Series},
year={2019},
volume={240},
pages={13}
}
• J. Labadie-Bartz, +58 authors G. Esquerdo
• Published 2019
• Physics
• Astrophysical Journal Supplement Series
• We present the discovery of KELT-22Ab, a hot Jupiter from the KELT-South survey. KELT-22Ab transits the moderately bright ($V\sim 11.1$) Sun-like G2V star TYC 7518-468-1. The planet has an orbital period of $P = 1.3866529 \pm 0.0000027$ days, a radius of $R_{P} = 1.285_{-0.071}^{+0.12}~R_{J}$, and a relatively large mass of $M_{P} = 3.47_{-0.14}^{+0.15}~ M_{J}$. The star has $R_{\star} = 1.099_{-0.046}^{+0.079}~ R_{\odot}$, $M_{\star} = 1.092_{-0.041}^{+0.045}~ M_{\odot}$, \${T_{\rm eff… CONTINUE READING
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