Issue |
A&A
Volume 623, March 2019
|
|
---|---|---|
Article Number | A100 | |
Number of page(s) | 8 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201834577 | |
Published online | 08 March 2019 |
A Jovian planet in an eccentric 11.5 day orbit around HD 1397 discovered by TESS
1
Geneva Observatory, University of Geneva,
Chemin des Mailettes 51,
1290
Versoix,
Switzerland
e-mail: Louise.Nielsen@unige.ch
2
Institute for Computational Science, University of Zurich,
Winterthurerstrasse 190,
8057
Zurich,
Switzerland
3
Department of Earth Sciences, University of California,
Riverside,
CA
92521,
USA
4
University of Southern Queensland,
Centre for Astrophysics,
Toowoomba,
QLD 4530,
Australia
5
SETI Institute,
Mountain View,
CA
94043,
USA
6
Proto-Logic LLC,
Washington,
DC
20009,
USA
7
Harvard-Smithsonian Center for Astrophysics,
60 Garden Street,
Cambridge,
MA
02138,
USA
8
Department of Physics and Kavli Institute for Astrophysics and Space Research, MIT,
Cambridge,
MA
02139,
USA
9
Department of Physics, Lehigh University,
16 Memorial Drive East,
Bethlehem,
PA
18015,
USA
10
Leidos/NASA Ames Research Center,
Moffett Field,
CA
94035,
USA
11
Department of Physics & Astronomy, Vanderbilt University,
6301 Stevenson Center Ln.,
Nashville,
TN
37235,
USA
12
Department of Earth, Atmospheric, and Planetary Sciences, and Department of Aeronautics and Astronautics, MIT,
77 Massachusetts Avenue,
Cambridge,
MA
02139,
USA
13
Department of Astrophysical Sciences, Princeton University,
4 Ivy Lane,
Princeton,
NJ
08544,
USA
14
NASA Ames Research Center,
Moffett Field,
CA
94035,
USA
15
Caltech/IPAC-NASA Exoplanet Science Institute,
M/S 100-22, 770 S. Wilson Ave,
Pasadena,
CA
91106,
USA
16
UC Santa Cruz, Department of Astronomy & Astrophysics,
1156 High Street,
Santa Cruz,
CA
95064,
USA
17
NASA Goddard Space Flight Center,
8800 Greenbelt Rd.,
Greenbelt,
MD
20771,
USA
18
Department of Astronomy, The University of Texas at Austin,
2515 Speedway C1400,
Austin,
TX
78712,
USA
19
Department of Physics and Astronomy, University of Louisville,
Louisville,
KY
40292,
USA
20
Astronomy Department, University of Florida,
211 Bryant Space Science Center, PO Box 112055,
Gainesville,
FL
32611-2055,
USA
21
Department of Physics and Astronomy, George Mason University,
Fairfax,
VA
22030,
USA
22
Exoplanetary Science at UNSW, School of Physics,
UNSW Sydney,
NSW 2052,
Australia
23
School of Astronomy and Space Science, Key Laboratory of Ministry of Education, Nanjing University,
Nanjing,
PR China
Received:
5
November
2018
Accepted:
18
February
2019
The Transiting Exoplanet Survey Satellite TESS has begun a new age of exoplanet discoveries around bright host stars. We present the discovery of HD 1397b (TOI-120.01), a giant planet in an 11.54-day eccentric orbit around a bright (V = 7.9) G-type subgiant. We estimate both host star and planetary parameters consistently using EXOFASTv2 based on TESS time-series photometry of transits and radial velocity measurements with CORALIE and MINERVA-Australis. We also present high angular resolution imaging with NaCo to rule out any nearby eclipsing binaries. We find that HD 1397b is a Jovian planet, with a mass of 0.415 ± 0.020 MJ and a radius of 1.026 ± 0.026 RJ. Characterising giant planets in short-period eccentric orbits, such as HD 1397b, is important for understanding and testing theories for the formation and migration of giant planets as well as planet-star interactions.
Key words: planets and satellites: detection / planets and satellites: individual: HD 1397b / planets and satellites: individual: TOI-120 / planets and satellites: individual: 394137592
© ESO 2019
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.