Modelling the HeI triplet absorption at 10 830 angstrom in the atmosphere of HD 209458 b

Abstract

Context. HD 209458 b is an exoplanet with an upper atmosphere undergoing blow-off escape that has mainly been studied using measurements of the Lyα absorption. Recently, high-resolution measurements of absorption in the He I triplet line at 10 830 Å of several exoplanets (including HD 209458 b) have been reported, creating a new opportunity to probe escaping atmospheres Aims. We aim to better understand the atmospheric regions of HD 209458 b from where the escape originates. Methods. We developed a 1D hydrodynamic model with spherical symmetry for the HD 209458 b thermosphere coupled with a nonlocal thermodynamic model for the population of the He I triplet state. In addition, we performed high-resolution radiative transfer calculations of synthetic spectra for the helium triplet lines and compared them with the measured absorption spectrum in order to retrieve information about the atmospheric parameters. Results. We find that the measured spectrum constrains the [H]/[H^(+) ] transition altitude occurring in the range of 1.2 R_(P)–1.9 R_(P). Hydrogen is almost fully ionised at altitudes above 2.9 R_(P). We also find that the X-ray and extreme ultraviolet absorption takes place at effective radii from 1.16 to 1.30 R_(P), and that the He I triplet peak density occurs at altitudes from 1.04 to 1.60 R_(P). Additionally, the averaged mean molecular weight is confined to the 0.61–0.73 g mole^(−1) interval, and the thermospheric H/He ratio should be larger than 90/10, and most likely approximately 98/2. We also provide a one-to-one relationship between mass-loss rate and temperature. Based on the energy-limited escape approach and assuming heating efficiencies of 0.1–0.2, we find a mass-loss rate in the range of (0.42–1.00) × 10^(11) g s^(−1) and a corresponding temperature range of 7125–8125 K. Conclusions. The analysis of the measured He I triplet absorption spectrum significantly constrains the thermospheric structure of HD 209458 b and advances our knowledge of its escaping atmosphere.