Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD 235088 b (TOI-1430 b) with CARMENES
Artikel i vetenskaplig tidskrift, 2023

HD 235088 (TOI-1430) is a young star known to host a sub-Neptune-sized planet candidate. We validated the planetary nature of HD 235088 b with multiband photometry, refined its planetary parameters, and obtained a new age estimate of the host star, placing it at 600- 800 Myr. Previous spectroscopic observations of a single transit detected an excess absorption of He I coincident in time with the planet candidate transit. Here, we confirm the presence of He I in the atmosphere of HD 235088 b with one transit observed with CARMENES. We also detected hints of variability in the strength of the helium signal, with an absorption of -0.91 ± 0.11%, which is slightly deeper (2γ) than the previous measurement. Furthermore, we simulated the He I signal with a spherically symmetric 1D hydrodynamic model, finding that the upper atmosphere of HD 235088 b escapes hydrodynamically with a significant mass loss rate of (1.5-5) × 1010 g s-1 in a relatively cold outflow, with T = 3125 ±375 K, in the photon-limited escape regime. HD 235088 b (Rp = 2.045 ± 0.075 R⊕) is the smallest planet found to date with a solid atmospheric detection - not just of He I but any other atom or molecule. This positions it a benchmark planet for further analyses of evolving young sub-Neptune atmospheres.

Planets and satellites: individual: HD 235088 b

Planets and satellites: atmospheres

Techniques: spectroscopic

Stars: individual: HD 235088

Techniques: photometric

Författare

J. Orell-Miquel

Universidad de la Laguna

Instituto de Astrofísica de Canarias

M. Lampon

Consejo Superior de Investigaciones Científicas (CSIC)

M. López-Puertas

Consejo Superior de Investigaciones Científicas (CSIC)

M. Mallorquín

Universidad de la Laguna

Instituto de Astrofísica de Canarias

F. Murgas

Instituto de Astrofísica de Canarias

Universidad de la Laguna

A. Peláez-Torres

Instituto de Astrofísica de Canarias

Universidad de la Laguna

Enric Palle

Instituto de Astrofísica de Canarias

Universidad de la Laguna

E. Esparza-Borges

Instituto de Astrofísica de Canarias

Universidad de la Laguna

J. Sanz-Forcada

European Space Astronomy Centre (ESAC)

H. M. Tabernero

Centro de Astrobiologia (CAB)

L. Nortmann

Georg-August-Universität Göttingen

E. Nagel

Georg-August-Universität Göttingen

H. Parviainen

Universidad de la Laguna

Instituto de Astrofísica de Canarias

M. Zapatero-Osorio

Centro de Astrobiologia (CAB)

J. A. Caballero

Centro de Astrobiologia (CAB)

S. Czesla

Thüringer Landessternwarte Tautenburg

C. Cifuentes

Centro de Astrobiologia (CAB)

Giuseppe Morello

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

Instituto de Astrofísica de Canarias

A. Quirrenbach

Landessternwarte Heidelberg-Königstuhl

P. J. Amado

Consejo Superior de Investigaciones Científicas (CSIC)

A. Fernández-Martín

Calar Alto Astronomical Observatory

A. Fukui

National Institutes of Natural Sciences

Instituto de Astrofísica de Canarias

T. Henning

Max-Planck-Gesellschaft

Kiyoe Kawauchi

University of Tokyo

Jerome P. De Leon

University of Tokyo

K. Molaverdikhani

Ludwig-Maximilians-Universität München (LMU)

Landessternwarte Heidelberg-Königstuhl

D. Montes

IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos)

Norio Narita

National Institutes of Natural Sciences

Instituto de Astrofísica de Canarias

University of Tokyo

A. Reiners

Georg-August-Universität Göttingen

I. Ribas

Consejo Superior de Investigaciones Científicas (CSIC)

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

A. Sánchez-López

Consejo Superior de Investigaciones Científicas (CSIC)

A. Schweitzer

Universität Hamburg

M. Stangret

Istituto nazionale di astrofisica (INAF)

F. Yan

University of Science and Technology of China

Astronomy and Astrophysics

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

Vol. 677 A56

Ämneskategorier (SSIF 2011)

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/202346445

Mer information

Senast uppdaterat

2025-03-09