Abstract
The future of exoplanet science is bright, as Transiting Exoplanet Survey Satellite (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 HD 21749b to be R ⊕, and combined archival and follow-up precision radial velocity data put the mass of the planet at M ⊕. HD 21749b contributes to the TESS Level 1 Science Requirement of providing 50 transiting planets smaller than 4 R ⊕ with measured masses. Furthermore, we report the discovery of HD 21749c (TOI 186.02), the first Earth-sized () planet from TESS. The HD 21749 system is a prime target for comparative studies of planetary composition and architecture in multi-planet systems.
Original language | English (US) |
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Article number | L7 |
Journal | Astrophysical Journal Letters |
Volume | 875 |
Issue number | 2 |
DOIs | |
State | Published - Apr 20 2019 |
Externally published | Yes |
Bibliographical note
Publisher Copyright:© 2019. The American Astronomical Society. All rights reserved..
Keywords
- planetary systems
- planets and satellites: detection
- stars: individual (HD 21749, TIC 279741379)