Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815
Journal article, 2024

We present the discovery and characterization of two warm mini-Neptunes transiting the K3V star TOI-815 in a K–M binary system. Analysis of its spectra and rotation period reveal the star to be young, with an age of 200+−400200 Myr. TOI-815b has a 11.2-day period and a radius of 2.94 ± 0.05 R+ with transits observed by TESS, CHEOPS, ASTEP, and LCOGT. The outer planet, TOI-815c, has a radius of 2.62 ± 0.10 R+, based on observations of three nonconsecutive transits with TESS; targeted CHEOPS photometry and radial velocity follow-up with ESPRESSO were required to confirm the 35-day period. ESPRESSO confirmed the planetary nature of both planets and measured masses of 7.6 ± 1.5 M+ (ρP = 1.64+−003331 g cm−3) and 23.5 ± 2.4 M+ (ρP = 7.2+−1110 g cm−3), respectively. Thus, the planets have very different masses, which is unusual for compact multi-planet systems. Moreover, our statistical analysis of mini-Neptunes orbiting FGK stars suggests that weakly irradiated planets tend to have higher bulk densities compared to those undergoing strong irradiation. This could be ascribed to their cooler atmospheres, which are more compressed and denser. Internal structure modeling of TOI-815b suggests it likely has a H-He atmosphere that constitutes a few percent of the total planet mass, or higher if the planet is assumed to have no water. In contrast, the measured mass and radius of TOI-815c can be explained without invoking any atmosphere, challenging planetary formation theories. Finally, we infer from our measurements that the star is viewed close to pole-on, which implies a spin-orbit misalignment at the 3σ level. This emphasizes the peculiarity of the system’s orbital architecture, and probably hints at an eventful dynamical history.

techniques: radial velocities

techniques: photometric

planets and satellites: composition

stars: individual: TOI-815

planets and satellites: detection

planets and satellites: formation

Author

A. Psaridi

University of Geneva

H. P. Osborn

University of Bern

F. Bouchy

University of Geneva

M. Lendl

University of Geneva

Léna Parc

University of Geneva

N. Billot

University of Geneva

C. Broeg

University of Bern

S.G. Sousa

University of Porto

V. Adibekyan

University of Porto

Omar Attia

University of Geneva

A. Bonfanti

Institut fur Weltraumforschung

Hritam Chakraborty

University of Geneva

Karen A. Collins

Harvard-Smithsonian Center for Astrophysics

Jeanne Davoult

University of Bern

E. Delgado Mena

University of Porto

N. Grieves

University of Geneva

T. Guillot

Observatoire de la Cote d'Azur

A. Heitzmann

University of Geneva

R. Helled

University of Zürich

Coel Hellier

Keele University

Jon M. Jenkins

NASA Ames Research Center

Henrik Knierim

University of Zürich

A. Krenn

Institut fur Weltraumforschung

Jack J. Lissauer

NASA Ames Research Center

R. Luque

University of Chicago

D. Rapetti

NASA Ames Research Center

N. C. Santos

University of Porto

Olga Suárez

Observatoire de la Cote d'Azur

J. Venturini

University of Geneva

Francis P. Wilkin

Union College

T.G. Wilson

The University of Warwick

J. N. Winn

Princeton University

C. Ziegler

Stephen F. Austin State University

Tiziano Zingales

University of Padua

Y. Alibert

University of Bern

A. Brandeker

Stockholm University

J. A. Egger

University of Bern

D. Gandolfi

University of Turin

M.J. Hooton

University of Cambridge

A. Tuson

University of Cambridge

S. Ulmer-Moll

University of Geneva

L. Abe

Observatoire de la Cote d'Azur

R. Allart

Université de Montréal

R. Alonso

Instituto de Astrofísica de Canarias

D. Anderson

The University of Warwick

G. A. Escudé

Institute of Space Sciences (ICE) - CSIC

T. Bárczy

Admatis

D. Barrado

Centro de Astrobiologia (CAB)

S.C.C. Barros

University of Porto

W. Baumjohann

Institut fur Weltraumforschung

M. Beck

University of Geneva

T. Beck

University of Bern

W. Benz

University of Bern

X. Bonfils

Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)

L. Borsato

Istituto nazionale di astrofisica (INAF)

V. Bourrier

University of Geneva

D. R. Ciardi

California Institute of Technology (Caltech)

A. Collier Cameron

University of St Andrews

S. Charnoz

Institut de Physique du Globe de Paris

M. Cointepas

University of Geneva

Szilard Csizmadia

German Aerospace Center (DLR)

P. E. Cubillos

Institut fur Weltraumforschung

G. Lo Curto

European Southern Observatory Santiago

M. B. Davies

Lund University

Tansu Daylan

Washington University in St. Louis

M. Deleuil

Laboratoire d'Astrophysique de Marseille

A. Deline

University of Geneva

L. Delrez

University of Liège

O. Demangeon

University of Porto

B.O. Demory

University of Bern

C. Dorn

Swiss Federal Institute of Technology in Zürich (ETH)

X. Dumusque

University of Geneva

D. Ehrenreich

University of Geneva

Anders Erikson

German Aerospace Center (DLR)

A. L. des Etangs

Institut d 'Astrophysique de Paris

D. de Miguel

Airbus Group

A. Fortier

University of Bern

L. Fossati

Institut fur Weltraumforschung

Yolanda G.C. Frensch

University of Geneva

Malcolm Fridlund

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Leiden University

Michaël Gillon

University of Liège

M. Gudel

University of Vienna

Maximilian N. Günther

European Space Research and Technology Centre (ESA ESTEC)

J. Hagelberg

University of Geneva

Ch. Helling

Institut fur Weltraumforschung

S. Hoyer

Laboratoire d'Astrophysique de Marseille

K. Isaak

European Space Research and Technology Centre (ESA ESTEC)

L. L. Kiss

Hungarian Academy of Sciences

K. W.F. Lam

German Aerospace Center (DLR)

J. Laskar

Paris Observatory

B. Lavie

University of Geneva

C. Lovis

University of Geneva

D. Magrin

Istituto nazionale di astrofisica (INAF)

L. Marafatto

Istituto nazionale di astrofisica (INAF)

P. Maxted

Keele University

S. McDermott

Protologic LLC

Djamel Mékarnia

Observatoire de la Cote d'Azur

C. Mordasini

University of Bern

F. Murgas

University of La Laguna

Valerio Nascimbeni

Istituto nazionale di astrofisica (INAF)

L. D. Nielsen

European Southern Observatory (ESO)

G. Olofsson

Stockholm University

R. Ottensamer

University of Vienna

I. Pagano

Istituto nazionale di astrofisica (INAF)

Enric Palle

Instituto de Astrofísica de Canarias

G. Peter

German Aerospace Center (DLR)

Giampaolo P. Piotto

University of Padua

Don L. Pollacco

The University of Warwick

D. Queloz

University of Cambridge

Roberto Ragazzoni

University of Padua

Devin Ramos

Union College

N. Rando

European Space Research and Technology Centre (ESA ESTEC)

H. Rauer

German Aerospace Center (DLR)

C. Reimers

University of Vienna

I. Ribas

Institute of Space Sciences (ICE) - CSIC

S. Seager

Massachusetts Institute of Technology (MIT)

D. Segransan

University of Geneva

Gaetano Scandariato

Istituto nazionale di astrofisica (INAF)

A.E. Simon

University of Bern

A. M.S. Smith

German Aerospace Center (DLR)

M. Stalport

University of Liège

Manfred B. Steller

Institut fur Weltraumforschung

G.M. Szabó

Eötvös Loránd University (ELTE)

Nicolas Thomas

University of Bern

T. Pritchard

NASA Goddard Space Flight Center

S. Udry

University of Geneva

C. Corral Van Damme

European Space Research and Technology Centre (ESA ESTEC)

V. Van Grootel

University of Liège

E. Villaver

Instituto de Astrofísica de Canarias

I. Walter

German Aerospace Center (DLR)

N. A. Walton

University of Cambridge

Cristilyn N. Watkins

Harvard-Smithsonian Center for Astrophysics

Richard G West

The University of Warwick

Astronomy and Astrophysics

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

Vol. 685 A5

Subject Categories

Meteorology and Atmospheric Sciences

Astronomy, Astrophysics and Cosmology

DOI

10.1051/0004-6361/202348678

More information

Latest update

7/2/2024 5