HIP 41378 observed by CHEOPS: Where is planet d?
Artikel i vetenskaplig tidskrift, 2024

HIP 41378 d is a long-period planet that has only been observed to transit twice, three years apart, with K2. According to stability considerations and a partial detection of the Rossiter- McLaughlin effect, Pd = 278.36 d has been determined to be the most likely orbital period. We targeted HIP 41378 d with CHEOPS at the predicted transit timing based on Pd = 278.36 d, but the observations show no transit. We find that large (> 22.4 h) transit timing variations (TTVs) could explain this non-detection during the CHEOPS observation window. We also investigated the possibility of an incorrect orbital solution, which would have major implications for our knowledge of this system. If Pd ≠ 278.36 d, the periods that minimize the eccentricity would be 101.22 d and 371.14 d. The shortest orbital period will be tested by TESS, which will observe HIP 41378 in Sector 88 starting in January 2025. Our study shows the importance of a mission like CHEOPS, which today is the only mission able to make long observations (i.e., from space) to track the ephemeris of long-period planets possibly affected by large TTVs.

HIP 41378

Planets and satellites

individual

Författare

S. Sulis

Laboratoire d'Astrophysique de Marseille

L. Borsato

Istituto nazionale di astrofisica (INAF)

S. Grouffal

Laboratoire d'Astrophysique de Marseille

H. P. Osborn

Massachusetts Institute of Technology (MIT)

Universität Bern

A. Santerne

Laboratoire d'Astrophysique de Marseille

A. Brandeker

Stockholms universitet

Maximilian N. Günther

European Space Research and Technology Centre (ESA ESTEC)

A. Heitzmann

Université de Genève

M. Lendl

Université de Genève

Malcolm Fridlund

Universiteit Leiden

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

D. Gandolfi

Universita degli Studi di Torino

Y. Alibert

Universität Bern

R. Alonso

Instituto de Astrofísica de Canarias

Universidad de la Laguna

T. Bárczy

Admatis

D. Barrado Navascues

European Space Astronomy Centre (ESAC)

S.C.C. Barros

Universidade do Porto

W. Baumjohann

Institut fur Weltraumforschung

T. Beck

Universität Bern

W. Benz

Universität Bern

M. Bergomi

Istituto nazionale di astrofisica (INAF)

N. Billot

Université de Genève

A. Bonfanti

Institut fur Weltraumforschung

C. Broeg

Universität Bern

A. Collier Cameron

University of St Andrews

C. Corral Van Damme

European Space Research and Technology Centre (ESA ESTEC)

A. Correia

Centre for Physics of the University of Coimbra

Szilard Csizmadia

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

P. E. Cubillos

Institut fur Weltraumforschung

Istituto nazionale di astrofisica (INAF)

M. B. Davies

Lunds universitet

M. Deleuil

Laboratoire d'Astrophysique de Marseille

A. Deline

Université de Genève

L. Delrez

Universite de Liège

KU Leuven

O. Demangeon

Universidade do Porto

B.O. Demory

Universität Bern

A. Derekas

Eötvös Loránd University (ELTE)

Billy Edwards

Netherlands Institute for Space Research (SRON)

D. Ehrenreich

Université de Genève

Anders Erikson

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

A. Fortier

Universität Bern

L. Fossati

Institut fur Weltraumforschung

K. Gazeas

University of Athens

Michaël Gillon

Universite de Liège

M. Gudel

Universität Wien

Ch. Helling

Technische Universität Graz

Institut fur Weltraumforschung

S. Hoyer

Laboratoire d'Astrophysique de Marseille

K. Isaak

European Space Research and Technology Centre (ESA ESTEC)

L. L. Kiss

Eötvös Loránd University (ELTE)

Magyar Tudomanyos Akademia

Judith Korth

Lunds universitet

K. W.F. Lam

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

J. Laskar

Observatoire de Paris

A. L. des Etangs

Institut d 'Astrophysique de Paris

D. Magrin

Istituto nazionale di astrofisica (INAF)

P. Maxted

Keele University

C. Mordasini

Universität Bern

Valerio Nascimbeni

Istituto nazionale di astrofisica (INAF)

G. Olofsson

Stockholms universitet

R. Ottensamer

Universität Wien

I. Pagano

Istituto nazionale di astrofisica (INAF)

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

Università di Padova

Istituto nazionale di astrofisica (INAF)

Don L. Pollacco

The University of Warwick

D. Queloz

Eidgenössische Technische Hochschule Zürich (ETH)

University of Cambridge

Roberto Ragazzoni

Università di Padova

Istituto nazionale di astrofisica (INAF)

N. Rando

European Space Research and Technology Centre (ESA ESTEC)

H. Rauer

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

Freie Universität Berlin

I. Ribas

Institut d'Estudis Espacials de Catalunya (IEEC)

Institut de Ciències de l'Espai (ICE) - CSIC

N. C. Santos

Universidade do Porto

Gaetano Scandariato

Istituto nazionale di astrofisica (INAF)

D. Segransan

Université de Genève

A.E. Simon

Universität Bern

A. M.S. Smith

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

S.G. Sousa

Universidade do Porto

M. Stalport

Universite de Liège

M. Steinberger

Institut fur Weltraumforschung

Gy M. Szabó

Eötvös Loránd University (ELTE)

A. Tuson

University of Cambridge

S. Udry

Université de Genève

S. Ulmer-Moll

Université de Genève

V. Van Grootel

Universite de Liège

J. Venturini

Université de Genève

E. Villaver

Universidad de la Laguna

Instituto de Astrofísica de Canarias

N. A. Walton

University of Cambridge

T.G. Wilson

The University of Warwick

D. Wolter

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

Tiziano Zingales

Università di Padova

Istituto nazionale di astrofisica (INAF)

Astronomy and Astrophysics

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

Vol. 686 L18

Ämneskategorier

Astronomi, astrofysik och kosmologi

Annan fysik

DOI

10.1051/0004-6361/202449689

Mer information

Senast uppdaterat

2024-08-21