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Verfasst von:Orell-Miquel, Jaume [VerfasserIn]   i
 Murgas, F. [VerfasserIn]   i
 Pallé, E. [VerfasserIn]   i
 Lampón, M. [VerfasserIn]   i
 López-Puertas, M. [VerfasserIn]   i
 Sanz-Forcada, J. [VerfasserIn]   i
 Nagel, E. [VerfasserIn]   i
 Kaminski, Adrian [VerfasserIn]   i
 Casasayas-Barris, N. [VerfasserIn]   i
 Nortmann, L. [VerfasserIn]   i
 Luque, R. [VerfasserIn]   i
 Molaverdikhani, Karan [VerfasserIn]   i
 Sedaghati, E. [VerfasserIn]   i
 Caballero, J. A. [VerfasserIn]   i
 Amado, P. J. [VerfasserIn]   i
 Bergond, G. [VerfasserIn]   i
 Czesla, S. [VerfasserIn]   i
 Hatzes, A. P. [VerfasserIn]   i
 Henning, Thomas [VerfasserIn]   i
 Khalafinejad, Sara [VerfasserIn]   i
 Montes, D. [VerfasserIn]   i
 Morello, G. [VerfasserIn]   i
 Quirrenbach, Andreas [VerfasserIn]   i
 Reiners, A. [VerfasserIn]   i
 Ribas, I. [VerfasserIn]   i
 Sánchez-López, A. [VerfasserIn]   i
 Schweitzer, A. [VerfasserIn]   i
 Stangret, M. [VerfasserIn]   i
 Yan, F. [VerfasserIn]   i
 Osorio, M. R. Zapatero [VerfasserIn]   i
Titel:A tentative detection of He I in the atmosphere of GJ 1214 b
Verf.angabe:J. Orell-Miquel, F. Murgas, E. Pallé, M. Lampón, M. López-Puertas, J. Sanz-Forcada, E. Nagel, A. Kaminski, N. Casasayas-Barris, L. Nortmann, R. Luque, K. Molaverdikhani, E. Sedaghati, J.A. Caballero, P.J. Amado, G. Bergond, S. Czesla, A.P. Hatzes, Th. Henning, S. Khalafinejad, D. Montes, G. Morello, A. Quirrenbach, A. Reiners, I. Ribas, A. Sánchez-López, A. Schweitzer, M. Stangret, F. Yan, and M.R. Zapatero Osorio
E-Jahr:2022
Jahr:04 March 2022
Umfang:12 S.
Fussnoten:Gesehen am 13.04.2022
Titel Quelle:Enthalten in: Astronomy and astrophysics
Ort Quelle:Les Ulis : EDP Sciences, 1969
Jahr Quelle:2022
Band/Heft Quelle:659(2022), Artikel-ID A55, Seite 1-12
ISSN Quelle:1432-0746
Abstract:The He I λ 10833 Å triplet is a powerful tool for characterising the upper atmosphere of exoplanets and tracing possible mass loss. Here, we analysed one transit of GJ 1214 b observed with the CARMENES high-resolution spectrograph to study its atmosphere via transmission spectroscopy around the He I triplet. Although previous studies using lower resolution instruments have reported non-detections of He I in the atmosphere of GJ 1214 b, we report here the first potential detection. We reconcile the conflicting results arguing that previous transit observations did not present good opportunities for the detection of He I, due to telluric H<sub>2<sub/>O absorption and OH emission contamination. We simulated those earlier observations, and show evidence that the planetary signal was contaminated. From our single non-telluric-contaminated transit, we determined an excess absorption of 2.10 % (4.6 <i>σ<i/>) with a full width at half maximum (FWHM) of 1.30 Å. The detection of He I is statistically significant at the 4.6 <i>σ<i/> level, but repeatability of the detection could not be confirmed due to the availability of only one transit. By applying a hydrodynamical model and assuming an H/He composition of 98/2, we found that GJ 1214 b would undergo hydrodynamic escape in the photon-limited regime, losing its primary atmosphere with a mass-loss rate of (1.5-18) × 10<sup>10<sup/> g s<sup>−1<sup/> and an outflow temperature in the range of 2900-4400 K. Further high-resolution follow-up observations of GJ 1214 b are needed to confirm and fully characterise the detection of an extended atmosphere surrounding GJ 1214 b. If confirmed, this would be strong evidence that this planet has a primordial atmosphere accreted from the original planetary nebula. Despite previous intensive observations from space- and ground-based observatories, our He I excess absorption is the first tentative detection of a chemical species in the atmosphere of this benchmark sub-Neptune planet
DOI:doi:10.1051/0004-6361/202142455
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext ; Verlag: https://doi.org/10.1051/0004-6361/202142455
 Volltext: https://www.aanda.org/articles/aa/abs/2022/03/aa42455-21/aa42455-21.html
 DOI: https://doi.org/10.1051/0004-6361/202142455
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1799512703
Verknüpfungen:→ Zeitschrift

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