A CHEOPS-enhanced view of the HD 3167 system
Artikel i vetenskaplig tidskrift, 2022

Much remains to be understood about the nature of exoplanets smaller than Neptune, most of which have been discovered in compact multi-planet systems. With its inner ultra-short period planet b aligned with the star and two larger outer planets d-c on polar orbits, the multi-planet system HD 3167 features a peculiar architecture and offers the possibility to investigate both dynamical and atmospheric evolution processes. To this purpose we combined multiple datasets of transit photometry and radial velocimetry (RV) to revise the properties of the system and inform models of its planets. This effort was spearheaded by CHEOPS observations of HD 3167b, which appear inconsistent with a purely rocky composition despite its extreme irradiation. Overall the precision on the planetary orbital periods are improved by an order of magnitude, and the uncertainties on the densities of the transiting planets b and c are decreased by a factor of 3. Internal structure and atmospheric simulations draw a contrasting picture between HD 3167d, likely a rocky super-Earth that lost its atmosphere through photo-evaporation, and HD 3167c, a mini-Neptune that kept a substantial primordial gaseous envelope. We detect a fourth, more massive planet on a larger orbit, likely coplanar with HD 3167d-c. Dynamical simulations indeed show that the outer planetary system d-c-e was tilted, as a whole, early in the system history, when HD 3167b was still dominated by the star influence and maintained its aligned orbit. RV data and direct imaging rule out that the companion that could be responsible for the present-day architecture is still bound to the HD 3167 system. Similar global studies of multi-planet systems will tell how many share the peculiar properties of the HD 3167 system, which remains a target of choice for follow-up observations and simulations.

Techniques: photometric

Planets and satellites: individual: HD 3167

Planets and satellites: dynamical evolution and stability

Planet-star interactions

Techniques: radial velocities

Planets and satellites: physical evolution

Författare

V. Bourrier

Université de Genève

A. Deline

Université de Genève

A. Krenn

Institut fur Weltraumforschung

J. A. Egger

Universität Bern

A. C. Petit

Köpenhamns universitet

L. Malavolta

Istituto nazionale di astrofisica (INAF)

Università di Padova

M. Cretignier

Université de Genève

N. Billot

Université de Genève

C. Broeg

Universität Bern

H.-G. Florén

Stockholms universitet

D. Queloz

Eidgenössische Technische Hochschule Zürich (ETH)

University of Cambridge

Y. Alibert

Universität Bern

A. Bonfanti

Institut fur Weltraumforschung

A. S. Bonomo

Istituto nazionale di astrofisica (INAF)

J. B. Delisle

Université de Genève

O. Demangeon

Universidade do Porto

B.O. Demory

Universität Bern

X. Dumusque

Université de Genève

D. Ehrenreich

Université de Genève

R. D. Haywood

University of Cambridge

S.B. Howell

NASA Ames Research Center

M. Lendl

Université de Genève

A. Mortier

University of Cambridge

G. Nigro

Università di Padova

Istituto nazionale di astrofisica (INAF)

S. Salmon

Université de Genève

S.G. Sousa

Universidade do Porto

T.G. Wilson

University of St Andrews

V. Adibekyan

Universidade do Porto

University of St Andrews

R. Alonso

Universidad de la Laguna

Instituto de Astrofísica de Canarias

G. Anglada

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

Institut d'Estudis Espacials de Catalunya (IEEC)

T. Bárczy

Admatis

D. Barrado

Centro de Astrobiologia (CAB)

S.C.C. Barros

Universidade do Porto

W. Baumjohann

Institut fur Weltraumforschung

M. Beck

Université de Genève

W. Benz

Universität Bern

F. Biondi

Istituto nazionale di astrofisica (INAF)

X. Bonfils

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

A. Brandeker

Stockholms universitet

J. Cabrera

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

S. Charnoz

Institut de Physique du Globe de Paris

Szilard Csizmadia

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

A. Collier Cameron

University of St Andrews

Mario Damasso

University of Exeter

M. B. Davies

Lunds universitet

M. Deleuil

Laboratoire d'Astrophysique de Marseille

L. Delrez

Universite de Liège

L. Di Fabrizio

Istituto nazionale di astrofisica (INAF)

Anders Erikson

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

A. Fortier

Universität Bern

L. Fossati

Institut fur Weltraumforschung

Malcolm Fridlund

Universiteit Leiden

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

D. Gandolfi

Universita degli Studi di Torino

Michaël Gillon

Universite de Liège

M. Gudel

Universität Wien

Kevin Heng

The University of Warwick

Universität Bern

S. Hoyer

Laboratoire d'Astrophysique de Marseille

K. Isaak

European Space Research and Technology Centre (ESA ESTEC)

L. Kiss

Magyar Tudomanyos Akademia

Eötvös Loránd University (ELTE)

J. Laskar

Observatoire de Paris

A. L. des Etangs

Institut d 'Astrophysique de Paris

V. Lorenzi

Instituto de Astrofísica de Canarias

Istituto nazionale di astrofisica (INAF)

C. Lovis

Université de Genève

D. Magrin

Istituto nazionale di astrofisica (INAF)

A. Massa

Universita degli Studi di Torino

P. Maxted

Keele University

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)

Giampaolo P. Piotto

Università di Padova

Istituto nazionale di astrofisica (INAF)

Don L. Pollacco

The University of Warwick

Roberto Ragazzoni

Istituto nazionale di astrofisica (INAF)

Università di Padova

N. Rando

European Space Research and Technology Centre (ESA ESTEC)

H. Rauer

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

Freie Universität Berlin

Technische 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

Alexis M. S. Smith

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

Manfred B. Steller

Institut fur Weltraumforschung

G.M. Szabó

Eötvös Loránd University (ELTE)

Nicolas Thomas

Universität Bern

S. Udry

Université de Genève

V. Van Grootel

Universite de Liège

F. Verrecchia

Osservatorio Astronomico di Roma

Agenzia Spaziale Italiana

N. A. Walton

University of Cambridge

T. Beck

Universität Bern

M. Buder

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

F. Ratti

European Space Research and Technology Centre (ESA ESTEC)

B. Ulmer

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

V. Viotto

Istituto nazionale di astrofisica (INAF)

Astronomy and Astrophysics

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

Vol. 668 A31

Ämneskategorier

Datorteknik

Astronomi, astrofysik och kosmologi

Inbäddad systemteknik

DOI

10.1051/0004-6361/202243778

Mer information

Senast uppdaterat

2023-09-15