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

Description
Summary: 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 (2<i>σ<i/>) 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) × 10<sup>10<sup/> g s<sup>−1<sup/> in a relatively cold outflow, with <i>T<i/> = 3125 ±375 K, in the photon-limited escape regime. HD 235088 b (<i>R<i/><sub>p<sub/> = 2.045 ± 0.075 <i>R<i/><sub>⊕<sub/>) 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.
Item Description: Gesehen am 23.04.2024
Online veröffentlicht: 05. September 2023
Physical Description: Illustrationen
17
ISSN: 1432-0746
DOI: 10.1051/0004-6361/202346445