dc.contributor.author
Morgado, B. E.
dc.contributor.author
Bruno, G.
dc.contributor.author
Gomes-Júnior, A. R.
dc.contributor.author
Pagano, I.
dc.contributor.author
Sicardy, B.
dc.contributor.author
Fortier, A.
dc.contributor.author
Desmars, J.
dc.contributor.author
Maxted, P. F. L.
dc.contributor.author
Braga-Ribas, F.
dc.contributor.author
Rauer, Heike
dc.date.accessioned
2022-11-14T10:53:32Z
dc.date.available
2022-11-14T10:53:32Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/36863
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-36576
dc.description.abstract
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.
en
dc.format.extent
9 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
methods: observational
en
dc.subject
techniques: photometric
en
dc.subject
occultations
en
dc.subject
minor planets
en
dc.subject
asteroids: individual: Quaoar
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
dc.title
A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.articlenumber
L15
dcterms.bibliographicCitation.doi
10.1051/0004-6361/202244221
dcterms.bibliographicCitation.journaltitle
Astronomy & Astrophysics
dcterms.bibliographicCitation.volume
664
dcterms.bibliographicCitation.url
https://doi.org/10.1051/0004-6361/202244221
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Planetologie und Fernerkundung
refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1432-0746
refubium.resourceType.provider
WoS-Alert