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TESS delivers its first Earth-sized planet and a warm sub-Neptune

Authors :
Todd C. Klaus
Xinyu Yao
Martin Paegert
Aylin Garcia Soto
Jim Francis
Keivan G. Stassun
Jennifer Burt
Jon M. Jenkins
Xavier Dumusque
Sara Seager
B. Scott Gaudi
Benjamin J. Fulton
Lizhou Sha
Steven Villanueva
Joseph E. Rodriguez
Elisabeth Matthews
Damien Ségransan
Avi Shporer
Sharon X. Wang
Timothy M. Brown
Stephen A. Shectman
Thomas G. Beatty
David James
Joshua Pepper
Jason D. Eastman
Francesco Pepe
Scott McDermott
Daniel J. Stevens
Andrew Vanderburg
Roland Vanderspek
R. Paul Butler
Joseph D. Twicken
Bill Wohler
Diana Dragomir
Johanna Teske
Zhuchang Zhan
David R. Ciardi
Christophe Lovis
Luca Fossati
Maximilian N. Günther
François Bouchy
Robert F. Goeke
David W. Latham
Joshua N. Winn
Chelsea X. Huang
Stéphane Udry
Michael B. Lund
George R. Ricker
Jeffrey D. Crane
Rudolf B. Kuhn
Robert J. Siverd
Publication Year :
2019
Publisher :
arXiv, 2019.

Abstract

The future of exoplanet science is bright, as TESS once again demonstrates with the discovery of its longest-period confirmed planet to date. We hereby present HD 21749b (TOI 186.01), a sub-Neptune in a 36-day orbit around a bright (V = 8.1) nearby (16 pc) K4.5 dwarf. TESS measures HD21749b to be 2.61$^{+0.17}_{-0.16}$ $R_{\oplus}$, and combined archival and follow-up precision radial velocity data put the mass of the planet at $22.7^{+2.2}_{-1.9}$ $M_{\oplus}$. HD 21749b contributes to the TESS Level 1 Science Requirement of providing 50 transiting planets smaller than 4 $R_{\oplus}$ with measured masses. Furthermore, we report the discovery of HD 21749c (TOI 186.02), the first Earth-sized ($R_p = 0.892^{+0.064}_{-0.058} R_{\oplus}$) planet from TESS. The HD21749 system is a prime target for comparative studies of planetary composition and architecture in multi-planet systems.<br />Comment: Published in ApJ Letters; 5 figures, 1 table

Details

Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....40b8afdd73ff6bc5ec758c16502c1c64
Full Text :
https://doi.org/10.48550/arxiv.1901.00051