A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS
Journal article, 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

Author

B. E. Morgado

Federal University of Rio de Janeiro

Lab Interinst E Astron LIneA

Observatorio Nacional

G. Bruno

Istituto nazionale di astrofisica (INAF)

A. R. Gomes-Junior

Lab Interinst E Astron LIneA

São Paulo State University (UNESP)

Federal University of Uberlândia

I Pagano

Istituto nazionale di astrofisica (INAF)

B. Sicardy

Paris Descartes University

A. Fortier

University of Bern

J. Desmars

Institute of Polytechnic Science and Aeronautics (IPSA)

University of Lille

P. F. L. Maxted

Keele University

F. Braga-Ribas

Lab Interinst E Astron LIneA

Observatorio Nacional

Federal University of Technology - Paraná

D. Queloz

University of Cambridge

Swiss Federal Institute of Technology in Zürich (ETH)

S. G. Sousa

University of Porto

J. L. Ortiz

Institute of Astrophysics of Andalusia (IAA)

A. Brandeker

Stockholm University

A. Collier Cameron

University of St Andrews

C. L. Pereira

Lab Interinst E Astron LIneA

Observatorio Nacional

H. G. Floren

Stockholm University

N. Hara

University of Geneva

D. Souami

Paris Descartes University

Laboratoire Joseph-Louis Lagrange

University of Namur

K. G. Isaak

European Space Research and Technology Centre (ESA ESTEC)

G. Olofsson

Stockholm University

P. Santos-Sanz

Institute of Astrophysics of Andalusia (IAA)

T. G. Wilson

University of St Andrews

J. Broughton

Reedy Creek Observatory

Trans Tasman Occultat Alliance TTOA

Y. Alibert

University of Bern

R. Alonso

Instituto de Astrofísica de Canarias

University of La Laguna

G. Anglada

Spanish National Research Council (CSIC)

Institute of Space Studies of Catalonia (IEEC)

T. Barczy

Admatis

D. Barrado

Spanish Astrobiology Center (INTA-CSIC)

S. C. C. Barros

University of Porto

W. Baumjohann

Austrian Academy of Sciences

M. Beck

University of Geneva

T. Beck

University of Bern

W. Benz

University of Bern

N. Billot

University of Geneva

X. Bonfils

Grenoble Alpes University

C. Broeg

University of Bern

J. Cabrera

German Aerospace Center (DLR)

S. Charnoz

Paris Descartes University

S. Csizmadia

German Aerospace Center (DLR)

M. B. Davies

Lund University

M. Deleuil

Aix Marseille University

L. Delrez

University of Liège

O. D. S. Demangeon

University of Porto

B. O. Demory

University of Bern

D. Ehrenreich

University of Geneva

A. Erikson

German Aerospace Center (DLR)

L. Fossati

Austrian Academy of Sciences

Malcolm Fridlund

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

D. Gandolfi

University of Turin

M. Gillon

University of Liège

M. Gudel

University of Vienna

K. Heng

University of Bern

The University of Warwick

S. Hoyer

Aix Marseille University

L. L. Kiss

Eötvös Loránd University (ELTE)

Hungarian Academy of Sciences

J. Laskar

Sorbonne University

A. Lecavelier des Etangs

Sorbonne University

M. Lendl

University of Geneva

C. Lovis

University of Geneva

D. Magrin

Istituto nazionale di astrofisica (INAF)

L. Marafatto

Istituto nazionale di astrofisica (INAF)

V Nascimbeni

Istituto nazionale di astrofisica (INAF)

R. Ottensamer

University of Vienna

E. Palle

Instituto de Astrofísica de Canarias

G. Peter

German Aerospace Center (DLR)

D. Piazza

University of Bern

G. Piotto

University of Padua

Istituto nazionale di astrofisica (INAF)

D. Pollacco

The University of Warwick

R. Ragazzoni

Istituto nazionale di astrofisica (INAF)

University of Padua

N. Rando

European Space Agency (ESA)

F. Ratti

European Space Agency (ESA)

H. Rauer

Technische Universität Berlin

Freie Universität Berlin

German Aerospace Center (DLR)

C. Reimers

University of Vienna

I Ribas

Spanish National Research Council (CSIC)

Institute of Space Studies of Catalonia (IEEC)

N. C. Santos

University of Porto

G. Scandariato

Istituto nazionale di astrofisica (INAF)

D. Segransan

University of Geneva

A. E. Simon

University of Bern

A. M. S. Smith

German Aerospace Center (DLR)

M. Steller

Austrian Academy of Sciences

G. M. Szabo

Eötvös Loránd University (ELTE)

N. Thomas

University of Bern

S. Udry

University of Geneva

V. Van Grootel

University of Liège

N. A. Walton

University of Cambridge

K. Westerdorff

German Aerospace Center (DLR)

Astronomy and Astrophysics

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

Vol. 664 L15

Exoplanet diversity with satellite studies

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

Subject Categories

Astronomy, Astrophysics and Cosmology

Other Physics Topics

Computer Vision and Robotics (Autonomous Systems)

DOI

10.1051/0004-6361/202244221

More information

Latest update

9/15/2023