Planet Hunters TESS III: two transiting planets around the bright G dwarf HD 152843

Author:

Eisner N L1ORCID,Nicholson B A12,Barragán O1ORCID,Aigrain S1,Lintott C1ORCID,Kaye L1,Klein B1ORCID,Miller G1,Taylor J1ORCID,Zicher N1,Buchhave L A3ORCID,Caldwell D A4,Horner J2,Llama J5,Mortier A67ORCID,Rajpaul V M6ORCID,Stassun K8ORCID,Sporer A9,Tkachenko A10,Jenkins J M11,Latham D12,Ricker G9,Seager S91314,Winn J15,Alhassan S16,Baeten E M L16,Bean S J16,Bundy D M16,Efremov V16,Ferstenou R16,Goodwin B L16,Hof M16,Hoffman T16,Hubert A16,Lau L16ORCID,Lee S16,Maetschke D16,Peltsch K1617,Rubio-Alfaro C16,Wilson G M16

Affiliation:

1. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK

2. Centre for Astrophysics, University of Southern Queensland, Toowoomba, Queensland 4350, Australia

3. DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 328, DK-2800 Kgs. Lyngby, Denmark

4. SETI Institute, 189 Bernardo Ave, Suite 200 Mountain View, CA 94043, USA

5. Lowell Observatory, 1400 W. Mars Hill Rd., Flagstaff, AZ 86001, USA

6. Astrophysics Group, Cavendish Laboratory, University of Cambridge, J.J. Thomson Avenue, Cambridge CB3 0HE, UK

7. Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

8. Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USA

9. Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

10. Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium

11. NASA Ames Research Center, Moffett Field, CA 94035, USA

12. Harvard–Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA

13. Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

14. Department of Aeronautics and Astronautics, MIT, 77 Massachusetts Avenue, Cambridge, MA 02139, USA

15. Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA

16. Citizen Scientist, Zooniverse c/o University of Oxford, Keble Road, Oxford OX1 3RH, UK

17. School of Computer Science & Technology, Algoma University, Sault Ste. Marie, ON P6A 2G4, Canada

Abstract

ABSTRACT We report on the discovery and validation of a two-planet system around a bright (V  = 8.85 mag) early G dwarf (1.43  R⊙, 1.15  M⊙, TOI 2319) using data from NASA’s Transiting Exoplanet Survey Satellite (TESS). Three transit events from two planets were detected by citizen scientists in the month-long TESS light curve (sector 25), as part of the Planet Hunters TESS project. Modelling of the transits yields an orbital period of $11.6264 _{ - 0.0025 } ^ { + 0.0022 }$ d and radius of $3.41 _{ - 0.12 } ^ { + 0.14 }$ R⊕ for the inner planet, and a period in the range 19.26–35 d and a radius of $5.83 _{ - 0.14 } ^ { + 0.14 }$ R⊕ for the outer planet, which was only seen to transit once. Each signal was independently statistically validated, taking into consideration the TESS light curve as well as the ground-based spectroscopic follow-up observations. Radial velocities from HARPS-N and EXPRES yield a tentative detection of planet b, whose mass we estimate to be $11.56 _{ - 6.14 } ^ { + 6.58 }$ M⊕, and allow us to place an upper limit of 27.5 M⊕ (99 per cent confidence) on the mass of planet c. Due to the brightness of the host star and the strong likelihood of an extended H/He atmosphere on both planets, this system offers excellent prospects for atmospheric characterization and comparative planetology.

Funder

NSF

Brinson Foundation

Moore Foundation

STFC

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. HD152843 b & c: the masses and orbital periods of a sub-Neptune and a superpuff Neptune;Monthly Notices of the Royal Astronomical Society;2024-07-26

2. The AstraLux-TESS high spatial resolution imaging survey;Astronomy & Astrophysics;2024-06

3. NIGHT: A compact, near-infrared, high-resolution spectrograph to survey helium in exoplanet systems;Monthly Notices of the Royal Astronomical Society;2023-10-26

4. A Recommendation to Retire VESPA for Exoplanet Validation;Research Notes of the AAS;2023-05-31

5. Three Long-period Transiting Giant Planets from TESS*;The Astronomical Journal;2023-05-04

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