The HD 93963 A transiting system: A 1.04d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS
Journal article, 2022

We present the discovery of two small planets transiting HD 93963A (TOI-1797), a GOV star (M-* = 1.109 +/- 0.043M(circle dot), R-* = 1.043 +/- 0.009 R-circle dot) in a visual binary system. We combined TESS and CHEOPS space-borne photometry with MuSCAT 2 ground-based photometry, 'Alopeke and PHARO high-resolution imaging, TRES and FIES reconnaissance spectroscopy, and SOPHIE radial velocity measurements. We validated and spectroscopically confirmed the outer transiting planet HD 93963 A c, a sub-Neptune with an orbital period of P-c approximate to 3.65 d that was reported to be a TESS object of interest (TOI) shortly after the release of Sector 22 data. HD 93963 A c has amass of M-c = 19.2 +/- 4.1 M-circle plus and a radius of R-c = 3.228 +/- 0.059 R-circle plus, implying a mean density of rho(c) = 3.1 +/- 0.7 g cm(-3). The inner object, HD 93963 A b, is a validated 1.04 d ultra-short period (USP) transiting super-Earth that we discovered in the TESS light curve and that was not listed as a TOI, owing to the low significance of its signal (TESS signal-to-noise ratio approximate to 6.7, TESS + CHEOPS combined transit depth D-b = 141.5(-8.3)(+8.5) ppm). We intensively monitored the star with CHEOPS by performing nine transit observations to confirm the presence of the inner planet and validate the system. HD 93963 A b is the first small (R-b = 1.35 +/- 0.042 R-circle plus) USP planet discovered and validated by TESS and CHEOPS. Unlike planet c, HD 93963 Ab is not significantly detected in our radial velocities (M-b = 7.8 +/- 3.2 M-circle plus). The two planets are on either side of the radius valley, implying that they could have undergone completely different evolution processes. We also discovered a linear trend in our Doppler measurements, suggesting the possible presence of a long-period outer planet. With a V-band magnitude of 9.2, HD 93963 A is among the brightest stars known to host a USP planet, making it one of the most favourable targets for precise mass measurement via Doppler spectroscopy and an important laboratory to test formation, evolution, and migration models of planetary systems hosting ultra-short period planets.

instrumentation: spectrographs

planets and satellites: detection

planets and satellites: fundamental parameters

instrumentation: photometers

methods: data analysis

Author

L. M. Serrano

University of Turin

D. Gandolfi

University of Turin

S. Hoyer

Aix Marseille University

A. Brandeker

Stockholm University

M. J. Hooton

University of Bern

S. Sousa

University of Porto

F. Murgas

University of La Laguna

Instituto de Astrofísica de Canarias

D. R. Ciardi

California Institute of Technology (Caltech)

S. B. Howell

NASA Ames Research Center

W. Benz

University of Bern

N. Billot

University of Geneva

H-G Floren

Stockholm University

A. Bekkelien

University of Geneva

A. Bonfanti

Austrian Academy of Sciences

A. Krenn

Austrian Academy of Sciences

Alexander James Mustill

Lund University

T. G. Wilson

University of St Andrews

H. Osborn

Massachusetts Institute of Technology (MIT)

University of Bern

H. Parviainen

Instituto de Astrofísica de Canarias

University of La Laguna

N. Heidari

Aix Marseille University

Université Nice Sophia Antipolis (UNS)

Shahid Beheshti University

E. Palle

University of La Laguna

Instituto de Astrofísica de Canarias

Malcolm Fridlund

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

V Adibekyan

University of Porto

L. Fossati

Austrian Academy of Sciences

M. Deleuil

Aix Marseille University

E. Knudstrup

Aarhus University

Nordic Optical Telescope

K. A. Collins

Harvard-Smithsonian Center for Astrophysics

K. W. F. Lam

German Aerospace Center (DLR)

S. Grziwa

University of Cologne

S. Salmon

University of Geneva

S. H. Albrecht

Aarhus University

Y. Alibert

University of Bern

R. Alonso

Instituto de Astrofísica de Canarias

University of La Laguna

G. Anglada-Escude

Institute of Space Studies of Catalonia (IEEC)

Spanish National Research Council (CSIC)

T. Barczy

Admatis

D. Barrado y Navascues

Spanish Astrobiology Center (INTA-CSIC)

S. C. C. Barros

University of Porto

W. Baumjohann

Austrian Academy of Sciences

M. Beck

University of Geneva

T. Beck

University of Bern

A. Bieryla

Harvard-Smithsonian Center for Astrophysics

X. Bonfils

Grenoble Alpes University

P. T. Boyd

NASA Goddard Space Flight Center

C. Broeg

University of Bern

J. Cabrera

German Aerospace Center (DLR)

S. Charnoz

Paris Descartes University

B. Chazelas

University of Geneva

J. L. Christiansen

California Institute of Technology (Caltech)

A. Collier Cameron

University of St Andrews

P. Cortes-Zuleta

Aix Marseille University

Sz Csizmadia

German Aerospace Center (DLR)

M. B. Davies

Lund University

A. Deline

University of Geneva

L. Delrez

University of Geneva

University of Liège

O. D. S. Demangeon

University of Porto

B-O Demory

University of Bern

A. Dunlavey

California Institute of Technology (Caltech)

University of California at Santa Cruz

D. Ehrenreich

University of Geneva

A. Erikson

German Aerospace Center (DLR)

A. Fortier

University of Bern

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

Z. Garai

Eötvös Loránd University (ELTE)

Slovak Academy of Sciences

M. Gillon

University of Liège

M. Gudel

University of Vienna

G. Hebrard

Pierre and Marie Curie University (UPMC)

Aix Marseille University

K. Heng

University of Bern

The University of Warwick

C. X. Huang

Massachusetts Institute of Technology (MIT)

K. G. Isaak

European Space Research and Technology Centre (ESA ESTEC)

J. M. Jenkins

NASA Ames Research Center

L. L. Kiss

Hungarian Academy of Sciences

J. Laskar

Sorbonne University

D. W. Latham

Harvard-Smithsonian Center for Astrophysics

A. Lecavelier des Etangs

Pierre and Marie Curie University (UPMC)

M. Lendl

University of Geneva

A. M. Levine

Massachusetts Institute of Technology (MIT)

C. Lovis

University of Geneva

M. B. Lund

California Institute of Technology (Caltech)

D. Magrin

Istituto nazionale di astrofisica (INAF)

P. F. L. Maxted

Keele University

N. Narita

Instituto de Astrofísica de Canarias

University of Tokyo

Astrobiology Center, Japan

V Nascimbeni

Istituto nazionale di astrofisica (INAF)

G. Olofsson

Stockholm University

R. Ottensamer

University of Vienna

I Pagano

Istituto nazionale di astrofisica (INAF)

Pessanha

Citizen Scientist

G. Peter

German Aerospace Center (DLR)

G. Piotto

University of Padua

Istituto nazionale di astrofisica (INAF)

D. Pollacco

The University of Warwick

D. Queloz

Swiss Federal Institute of Technology in Zürich (ETH)

University of Cambridge

R. Ragazzoni

Istituto nazionale di astrofisica (INAF)

University of Padua

N. Rando

European Space Agency (ESA)

F. Ratti

European Space Agency (ESA)

H. Rauer

German Aerospace Center (DLR)

Technische Universität Berlin

Freie Universität Berlin

I Ribas

Institute of Space Studies of Catalonia (IEEC)

Spanish National Research Council (CSIC)

G. Ricker

Massachusetts Institute of Technology (MIT)

P. Rowden

Royal Astronomical Society

N. C. Santos

University of Porto

G. Scandariato

Istituto nazionale di astrofisica (INAF)

S. Seager

Massachusetts Institute of Technology (MIT)

D. Segransan

University of Geneva

A. E. Simon

University of Bern

A. M. S. Smith

German Aerospace Center (DLR)

M. Steller

Austrian Academy of Sciences

Gy M. Szabo

Eötvös Loránd University (ELTE)

N. Thomas

University of Bern

J. D. Twicken

NASA Ames Research Center

S. Udry

University of Geneva

B. Ulmer

German Aerospace Center (DLR)

V. Van Grootel

University of Liège

R. Vanderspek

Massachusetts Institute of Technology (MIT)

V. Viotto

Istituto nazionale di astrofisica (INAF)

N. Walton

University of Cambridge

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 667 A1

Exoplanet diversity with satellite studies

Swedish National Space Board (174/18), 2019-02-04 -- 2023-08-01.

Subject Categories

Medical Laboratory and Measurements Technologies

Astronomy, Astrophysics and Cosmology

Signal Processing

DOI

10.1051/0004-6361/202243093

More information

Latest update

8/8/2024 2