2021A&A...653A..52F


Query : 2021A&A...653A..52F

2021A&A...653A..52F - Astronomy and Astrophysics, volume 653A, 52-52 (2021/9-1)

Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b.

FOSSATI L., YOUNG M.E., SHULYAK D., KOSKINEN T., HUANG C., CUBILLOS P.E., FRANCE K. and SREEJITH A.G.

Abstract (from CDS):


Context. Several observational and theoretical results indicate that the atmospheric temperature of the ultra-hot Jupiter KELT-9b in the main line formation region is a few thousand degrees higher than predicted by self-consistent models.
Aims. Our aim was to test whether non-local thermodynamic equilibrium (NLTE) effects are responsible for the presumably higher temperature.
Methods. We employed the Cloudy NLTE radiative transfer code to self-consistently compute the upper atmospheric temperature-pressure (TP) profile of KELT-9b, assuming solar metallicity and accounting for Roche potential. In the lower atmosphere, we used an updated version of the HELIOS radiative-convective equilibrium code to constrain the Cloudy model.
Results. The Cloudy NLTE TP profile is ≃2000K hotter than that obtained with previous models assuming LTE. In particular, in the 1-10–7bar range the temperature increases from ≃4000 to ≃8500K, remaining roughly constant at lower pressures. We find that the high temperature in the upper atmosphere of KELT-9b is driven principally by NLTE effects modifying the Fe and Mg level populations, which strongly influence the atmospheric thermal balance. We employed Cloudy to compute LTE and NLTE synthetic transmission spectra on the basis of the TP profiles computed in LTE and NLTE, respectively, finding that the NLTE model generally produces stronger absorption lines, particularly in the ultraviolet, than the LTE model (up to 30%). We compared the NLTE synthetic transmission spectrum with the observed Hα and Hβ line profiles obtaining an excellent match, thus supporting our results.
Conclusions. The NLTE synthetic transmission spectrum can be used to guide future observations aiming at detecting features in the KELT-9b transmission spectrum. Metals, such as Mg and Fe, and NLTE effects shape the upper atmospheric temperature structure of KELT-9b, and thus affect the mass-loss rates derived from it. Finally, our results call for checking whether this is the case also for cooler planets.

Abstract Copyright: © ESO 2021

Journal keyword(s): radiative transfer - planets and satellites: atmospheres - planets and satellites: gaseous planets - planets and satellites: individual: KELT-9b

Simbad objects: 6

goto Full paper

goto View the references in ADS

Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 BD+01 316b Pl 01 46 31.8575937456 +02 42 02.030065560           ~ 205 0
2 HD 15082b Pl 02 26 51.0582618096 +37 33 01.736482032           ~ 337 1
3 CD-38 3220b Pl 07 10 24.0604565856 -39 05 50.571250476           ~ 297 0
4 WASP-189b Pl? 15 02 44.8678907928 -03 01 52.986571896           ~ 82 0
5 HD 185603b Pl 19 38 38.7352230144 +31 13 09.217127532           ~ 127 0
6 HD 195689b Pl 20 31 26.3534153736 +39 56 19.773037500           ~ 278 0

To bookmark this query, right click on this link: simbad:objects in 2021A&A...653A..52F and select 'bookmark this link' or equivalent in the popup menu