A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS
Artikel i vetenskaplig tidskrift, 2022

Context. Stellar occultation is a powerful technique that allows the determination of some physical parameters of the occulting object. The result depends on the photometric accuracy, the temporal resolution, and the number of chords obtained. Space telescopes can achieve high photometric accuracy as they are not affected by atmospheric scintillation. Aims. Using ESA's CHEOPS space telescope, we observed a stellar occultation by the transneptunian object (50000) Quaoar. We compare the obtained chord with previous occultations by this object and determine its astrometry with sub-milliarcsecond precision. Also, we determine upper limits to the presence of a global methane atmosphere on the occulting body. Methods. We predicted and observed a stellar occultation by Quaoar using the CHEOPS space telescope. We measured the occultation light curve from this dataset and determined the dis- and reappearance of the star behind the occulting body. Furthermore, a ground-based telescope in Australia was used to constrain Quaoar's limb. Combined with results from previous works, these measurements allowed us to obtain a precise position of Quaoar at the occultation time. Results. We present the results obtained from the first stellar occultation by a transneptunian object using a space telescope orbiting Earth; it was the occultation by Quaoar observed on 2020 June 11. We used the CHEOPS light curve to obtain a surface pressure upper limit of 85 nbar for the detection of a global methane atmosphere. Also, combining this observation with a ground-based observation, we fitted Quaoar's limb to determine its astrometric position with an uncertainty below 1.0 mas. Conclusions. This observation is the first of its kind, and it shall be considered as a proof of concept of stellar occultation observations of transneptunian objects with space telescopes orbiting Earth. Moreover, it shows significant prospects for the James Webb Space Telescope.

minor planets, asteroids: individual: Quaoar

techniques: photometric

methods: observational

occultations

Författare

B. E. Morgado

Universidade Federal do Rio de Janeiro (UFRJ)

Lab Interinst E Astron LIneA

Observatorio Nacional

G. Bruno

Istituto nazionale di astrofisica (INAF)

A. R. Gomes-Junior

Lab Interinst E Astron LIneA

Universidade Estadual Paulista (UNESP)

Federal University of Uberlândia

I Pagano

Istituto nazionale di astrofisica (INAF)

B. Sicardy

Université Paris Descartes

A. Fortier

Universität Bern

J. Desmars

Institut Polytechnique des Sciences Avancées (IPSA)

Université de Lille

P. F. L. Maxted

Keele University

F. Braga-Ribas

Lab Interinst E Astron LIneA

Observatorio Nacional

Universidade Tecnologica Federal do Parana

D. Queloz

University of Cambridge

Eidgenössische Technische Hochschule Zürich (ETH)

S. G. Sousa

Universidade do Porto

J. L. Ortiz

Instituto de Astrofisica de Andalucía (IAA)

A. Brandeker

Stockholms universitet

A. Collier Cameron

University of St Andrews

C. L. Pereira

Lab Interinst E Astron LIneA

Observatorio Nacional

H. G. Floren

Stockholms universitet

N. Hara

Université de Genève

D. Souami

Université Paris Descartes

Laboratoire Joseph-Louis Lagrange

University of Namur

K. G. Isaak

European Space Research and Technology Centre (ESA ESTEC)

G. Olofsson

Stockholms universitet

P. Santos-Sanz

Instituto de Astrofisica de Andalucía (IAA)

T. G. Wilson

University of St Andrews

J. Broughton

Reedy Creek Observatory

Trans Tasman Occultat Alliance TTOA

Y. Alibert

Universität Bern

R. Alonso

Instituto de Astrofísica de Canarias

Universidad de la Laguna

G. Anglada

Consejo Superior de Investigaciones Científicas (CSIC)

Institut d'Estudis Espacials de Catalunya (IEEC)

T. Barczy

Admatis

D. Barrado

Centro de Astrobiología (INTA-CSIC)

S. C. C. Barros

Universidade do Porto

W. Baumjohann

Österreichische Akademie der Wissenschaften

M. Beck

Université de Genève

T. Beck

Universität Bern

W. Benz

Universität Bern

N. Billot

Université de Genève

X. Bonfils

Université Grenoble Alpes

C. Broeg

Universität Bern

J. Cabrera

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

S. Charnoz

Université Paris Descartes

S. Csizmadia

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

M. B. Davies

Lunds universitet

M. Deleuil

Aix-Marseille Université

L. Delrez

Universite de Liège

O. D. S. Demangeon

Universidade do Porto

B. O. Demory

Universität Bern

D. Ehrenreich

Université de Genève

A. Erikson

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

L. Fossati

Österreichische Akademie der Wissenschaften

Malcolm Fridlund

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

D. Gandolfi

Universita degli Studi di Torino

M. Gillon

Universite de Liège

M. Gudel

Universität Wien

K. Heng

Universität Bern

The University of Warwick

S. Hoyer

Aix-Marseille Université

L. L. Kiss

Eötvös Loránd University (ELTE)

Magyar Tudomanyos Akademia

J. Laskar

Sorbonne Université

A. Lecavelier des Etangs

Sorbonne Université

M. Lendl

Université de Genève

C. Lovis

Université de Genève

D. Magrin

Istituto nazionale di astrofisica (INAF)

L. Marafatto

Istituto nazionale di astrofisica (INAF)

V Nascimbeni

Istituto nazionale di astrofisica (INAF)

R. Ottensamer

Universität Wien

E. Palle

Instituto de Astrofísica de Canarias

G. Peter

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

D. Piazza

Universität Bern

G. Piotto

Università di Padova

Istituto nazionale di astrofisica (INAF)

D. Pollacco

The University of Warwick

R. Ragazzoni

Istituto nazionale di astrofisica (INAF)

Università di Padova

N. Rando

Europeiska rymdorganisationen (ESA)

F. Ratti

Europeiska rymdorganisationen (ESA)

H. Rauer

Technische Universität Berlin

Freie Universität Berlin

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

C. Reimers

Universität Wien

I Ribas

Consejo Superior de Investigaciones Científicas (CSIC)

Institut d'Estudis Espacials de Catalunya (IEEC)

N. C. Santos

Universidade do Porto

G. 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)

M. Steller

Österreichische Akademie der Wissenschaften

G. M. Szabo

Eötvös Loránd University (ELTE)

N. Thomas

Universität Bern

S. Udry

Université de Genève

V. Van Grootel

Universite de Liège

N. A. Walton

University of Cambridge

K. Westerdorff

Deutsches Zentrums für Luft- und Raumfahrt (DLR)

Astronomy and Astrophysics

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

Vol. 664 L15

Satellitstudier av exoplaneters mångfald

Rymdstyrelsen (174/18), 2019-02-04 -- 2023-08-01.

Ämneskategorier

Astronomi, astrofysik och kosmologi

Annan fysik

Datorseende och robotik (autonoma system)

DOI

10.1051/0004-6361/202244221

Mer information

Senast uppdaterat

2023-09-15