Transit-timing variations in the AU Mic system observed with CHEOPS
Journal article, 2025

Context. AU Mic is a very active M dwarf star with an edge-on debris disk and two known transiting sub-Neptunes with a possible third planetary companion. The two transiting planets exhibit significant transit-timing variations (TTVs) that are caused by the gravi tational interaction between the bodies in the system. Aims. Using photometrical observations taken with the CHaracterizing ExOPlanet Satellite (CHEOPS), we aim to constrain the plan etary radii, the orbital distances, and the periods of AU Mic b and c. Furthermore, our goal is to determine the superperiod of the TTVs for AU Mic b and to update the transit ephemeris for both planets. Additionally, based on the perceived TTVs, we study the possible presence of a third planet in the system. Methods. We conducted ultra-high precision photometric observations with CHEOPS in 2022 and 2023. We used Allesfitter to fit the planetary transits and to constrain the planetary and orbital parameters. We combined our new measurements with results from previous years to determine the periods and amplitudes of the TTVs. We applied dynamical modelling based on TTV measurements from the 2018-2023 period to reconstruct the perceived variations. Results. We found that the orbital distances and periods for AU Mic b and c agree with the results from previous works. However, the values for the planetary radii deviate slightly from previous values, which we attribute to the effect of spots on the stellar surface. AU Mic c showed very strong TTVs, with transits that occurred ∼80 minutes later in 2023 than in 2021. Through a dynamical analysis of the system, we found that the observed TTVs can be explained by a third planet with an orbital period of ∼12.6 days and a mass of 0.2030.024+0.022 MO. We explored the orbital geometry of the system and found that AU Mic c has a misaligned retrograde orbit. The limited number of AU Mic observations prevented us from determining the exact dynamical configuration and planetary parameters. Further monitoring of the system with CHEOPS might help to improve these results.

Planets and satellites: fundamental parameters

Author

Boldog

Eötvös Loránd University (ELTE)

Research Centre For Astronomy and Earth Sciences

Hungarian Academy of Sciences

G.M. Szabó

Eötvös Loránd University (ELTE)

L. Kriskovics

Research Centre For Astronomy and Earth Sciences

Hungarian Academy of Sciences

L. Borsato

Istituto nazionale di astrofisica (INAF)

D. Gandolfi

University of Turin

M. Lendl

University of Geneva

Maximilian N. Günther

European Space Research and Technology Centre (ESA ESTEC)

A. Heitzmann

University of Geneva

T.G. Wilson

The University of Warwick

A. Brandeker

Stockholm University

Z. Garai

Eötvös Loránd University (ELTE)

Slovak Academy of Sciences

Y. Alibert

Physics Institute

University of Bern

R. Alonso

University of La Laguna

Instituto de Astrofísica de Canarias

T. Bárczy

Admatis

D. Barrado Navascues

Centro de Astrobiologia (CAB)

S.C.C. Barros

University of Porto

W. Baumjohann

Institut fur Weltraumforschung

W. Benz

Physics Institute

University of Bern

N. Billot

University of Geneva

C. Broeg

Physics Institute

University of Bern

A. Collier Cameron

University of St Andrews

A. Correia

Centre for Physics of the University of Coimbra

Szilard Csizmadia

German Aerospace Center (DLR)

P. E. Cubillos

Istituto nazionale di astrofisica (INAF)

Institut fur Weltraumforschung

Melvyn B. Davies

Lund University

M. Deleuil

Laboratoire d'Astrophysique de Marseille

A. Deline

University of Geneva

O. Demangeon

University of Porto

B.O. Demory

University of Bern

Physics Institute

A. Derekas

Eötvös Loránd University (ELTE)

Billy Edwards

Netherlands Institute for Space Research (SRON)

J. A. Egger

Physics Institute

D. Ehrenreich

University of Geneva

Anders Erikson

German Aerospace Center (DLR)

A. Fortier

University of Bern

Physics Institute

L. Fossati

Institut fur Weltraumforschung

Malcolm Fridlund

Leiden University

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

K. Gazeas

University of Athens

Michaël Gillon

University of Liège

M. Gudel

University of Vienna

P. Guterman

Laboratoire d'Astrophysique de Marseille

CS20330

Ch. Helling

Technische Universität Graz

Institut fur Weltraumforschung

K. Isaak

European Space Research and Technology Centre (ESA ESTEC)

L. L. Kiss

Eötvös Loránd University (ELTE)

Hungarian Academy of Sciences

E. Kopp

German Aerospace Center (DLR)

Judith Korth

Lund University

K. W.F. Lam

German Aerospace Center (DLR)

J. Laskar

Paris Observatory

A. L. des Etangs

Institut d 'Astrophysique de Paris

A. Luntzer

University of Vienna

D. Magrin

Istituto nazionale di astrofisica (INAF)

G. Mantovan

University of Padua

L. Marafatto

Istituto nazionale di astrofisica (INAF)

P. Maxted

Keele University

Bruno Merín

European Space Astronomy Centre (ESAC)

C. Mordasini

University of Bern

Physics Institute

M. Munari

Istituto nazionale di astrofisica (INAF)

Valerio Nascimbeni

Istituto nazionale di astrofisica (INAF)

G. Olofsson

Stockholm University

R. Ottensamer

University of Vienna

I. Pagano

Istituto nazionale di astrofisica (INAF)

Enric Palle

University of La Laguna

Instituto de Astrofísica de Canarias

G. Peter

German Aerospace Center (DLR)

D. Piazza

University of Bern

Giampaolo P. Piotto

University of Padua

Istituto nazionale di astrofisica (INAF)

Don L. Pollacco

The University of Warwick

K. Poppenhaeger

Leibniz Institute for Astrophysics Potsdam

D. Queloz

University of Cambridge

Swiss Federal Institute of Technology in Zürich (ETH)

Roberto Ragazzoni

Istituto nazionale di astrofisica (INAF)

University of Padua

N. Rando

European Space Research and Technology Centre (ESA ESTEC)

H. Rauer

Freie Universität Berlin

German Aerospace Center (DLR)

I. Ribas

Spanish National Research Council (CSIC)

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

M. Rieder

University of Bern

N. C. Santos

University of Porto

Gaetano Scandariato

Istituto nazionale di astrofisica (INAF)

D. Segransan

University of Geneva

A.E. Simon

University of Bern

Physics Institute

A. M.S. Smith

German Aerospace Center (DLR)

S.G. Sousa

University of Porto

R. Southworth

European Space Operations Centre

M. Stalport

University of Liège

S. Sulis

Laboratoire d'Astrophysique de Marseille

S. Udry

University of Geneva

S. Ulmer-Moll

University of Geneva

Physics Institute

University of Liège

V. Van Grootel

University of Liège

J. Venturini

University of Geneva

E. Villaver

Instituto de Astrofísica de Canarias

University of La Laguna

N. A. Walton

University of Cambridge

Tiziano Zingales

University of Padua

Istituto nazionale di astrofisica (INAF)

Astronomy and Astrophysics

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

Vol. 694 A137

Exoplanet diversity with satellite studies

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

Exoplanets from space – CHEOPS and PLATO, ESA’s next two projects

Swedish National Space Board (174/18), 2017-01-01 -- 2022-12-31.

Subject Categories (SSIF 2025)

Astronomy, Astrophysics, and Cosmology

DOI

10.1051/0004-6361/202452699

More information

Latest update

3/9/2025 1