The changing face of AU Mic b: Stellar spots, spin-orbit commensurability, and transit timing variations as seen by CHEOPS and TESS
Artikel i vetenskaplig tidskrift, 2021
AU Mic is a young planetary system with a resolved debris disc showing signs of planet formation and two transiting warm Neptunes near mean-motion resonances. Here we analyse three transits of AU Mic b observed with the CHaracterising ExOPlanet Satellite (CHEOPS), supplemented with sector 1 and 27 Transiting Exoplanet Survey Satellite (TESS) photometry, and the All-Sky Automated Survey from the ground. The refined orbital period of AU Mic b is 8.462995 ± 0.000003 d, whereas the stellar rotational period is Prot = 4.8367 ± 0.0006 d. The two periods indicate a 7:4 spin-orbit commensurability at a precision of 0.1%. Therefore, all transits are observed in front of one of the four possible stellar central longitudes. This is strongly supported by the observation that the same complex star-spot pattern is seen in the second and third CHEOPS visits that were separated by four orbits (and seven stellar rotations). Using a bootstrap analysis we find that flares and star spots reduce the accuracy of transit parameters by up to 10% in the planet-to-star radius ratio and the accuracy on transit time by 3-4 min. Nevertheless, occulted stellar spot features independently confirm the presence of transit timing variations (TTVs) with an amplitude of at least 4 min. We find that the outer companion, AU Mic c, may cause the observed TTVs.
Planetary systems
Författare
G.M. Szabó
Eötvös Loránd University (ELTE)
D. Gandolfi
Istituto nazionale di astrofisica (INAF)
A. Brandeker
Stockholms universitet
Szilard Csizmadia
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
Z. Garai
Eötvös Loránd University (ELTE)
Slovenská akadémia Vied
N. Billot
Université de Genève
C. Broeg
Universität Bern
D. Ehrenreich
Université de Genève
A. Fortier
Universität Bern
L. Fossati
Institut fur Weltraumforschung
S. Hoyer
Laboratoire d'Astrophysique de Marseille
L. Kiss
Eötvös Loránd University (ELTE)
Magyar Tudomanyos Akademia
The University of Sydney
A. L. des Etangs
Institut d 'Astrophysique de Paris
P. Maxted
Keele University
I. Ribas
Institut de Ciències de l'Espai (ICE) - CSIC
Institut d'Estudis Espacials de Catalunya (IEEC)
Y. Alibert
Universität Bern
R. Alonso
Instituto de Astrofísica de Canarias
Universidad de la Laguna
G. A. Escudé
Institut de Ciències de l'Espai (ICE) - CSIC
Institut d'Estudis Espacials de Catalunya (IEEC)
T. Bárczy
Admatis
S.C.C. Barros
Universidade do Porto
D. Barrado
Centro de Astrobiologia (CAB)
W. Baumjohann
Institut fur Weltraumforschung
M. Beck
Université de Genève
T. Beck
Universität Bern
A. Bekkelien
Université de Genève
X. Bonfils
Université Grenoble Alpes
W. Benz
Universität Bern
L. Borsato
Osservatorio Astronomico di Padova
M.-D. Busch
Universität Bern
J. Cabrera
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
S. Charnoz
Institut de Physique du Globe de Paris
A. Collier Cameron
University of St Andrews
C. Corral Van Damme
European Space Research and Technology Centre (ESA ESTEC)
M. B. Davies
Lunds universitet
L. Delrez
Universite de Liège
M. Deleuil
Laboratoire d'Astrophysique de Marseille
O. Demangeon
Laboratoire d'Astrophysique de Marseille
Universidade do Porto
B.O. Demory
Universität Bern
Anders Erikson
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
Malcolm Fridlund
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Universiteit Leiden
D. Futyan
Université de Genève
A. Garciá Muñoz
Technische Universität Berlin
Michaël Gillon
Universite de Liège
M. Guedel
Universität Wien
P. Guterman
Institut National des Sciences de l'Univers
Laboratoire d'Astrophysique de Marseille
Kevin Heng
Universität Bern
The University of Warwick
K. Isaak
European Space Research and Technology Centre (ESA ESTEC)
G. Lacedelli
Osservatorio Astronomico di Padova
Università di Padova
J. Laskar
Observatoire de Paris
M. Lendl
Université de Genève
C. Lovis
Université de Genève
A. Luntzer
Universität Wien
D. Magrin
Osservatorio Astronomico di Padova
Valerio Nascimbeni
Osservatorio Astronomico di Padova
G. Olofsson
Stockholms universitet
H. P. Osborn
Universität Bern
Massachusetts Institute of Technology (MIT)
R. Ottensamer
Universität Wien
I. Pagano
Osservatorio Astrofisico di Catania
Enric Palle
Instituto de Astrofísica de Canarias
Universidad de la Laguna
G. Peter
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
D. Piazza
Universität Bern
Giampaolo P. Piotto
Osservatorio Astronomico di Padova
Università di Padova
Don L. Pollacco
The University of Warwick
D. Queloz
University of Cambridge
Université de Genève
Roberto Ragazzoni
Osservatorio Astronomico di Padova
Università di Padova
N. Rando
European Space Research and Technology Centre (ESA ESTEC)
H. Rauer
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
Technische Universität Berlin
Freie Universität Berlin
N. C. Santos
Universidade do Porto
Gaetano Scandariato
Osservatorio Astrofisico di Catania
D. Segransan
Université de Genève
L. M. Serrano
Universita degli Studi di Torino
D. Sicilia
Osservatorio Astrofisico di Catania
A.E. Simon
Universität Bern
Alexis M. S. Smith
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
S.G. Sousa
Universidade do Porto
Manfred B. Steller
Institut fur Weltraumforschung
Nicolas Thomas
Universität Bern
S. Udry
Université de Genève
V. Van Grootel
Universite de Liège
N. A. Walton
University of Cambridge
T.G. Wilson
University of St Andrews
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 654 A159Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
Den kondenserade materiens fysik
DOI
10.1051/0004-6361/202140345