2022MNRAS.509.5858H


Query : 2022MNRAS.509.5858H

2022MNRAS.509.5858H - Mon. Not. R. Astron. Soc., 509, 5858-5871 (2022/February-1)

The impact of coronal mass ejections and flares on the atmosphere of the hot Jupiter HD189733b.

HAZRA G., VIDOTTO A.A., CAROLAN S., VILLARREAL D'ANGELO C. and MANCHESTER W.

Abstract (from CDS):

High-energy stellar irradiation can photoevaporate planetary atmospheres, which can be observed in spectroscopic transits of hydrogen lines. For the exoplanet HD189733b, multiple observations in the Ly α line have shown that atmospheric evaporation is variable, going from undetected to enhanced evaporation in a 1.5-yr interval. Coincidentally or not, when HD189733b was observed to be evaporating, a stellar flare had just occurred 8 h prior to the observation. This led to the question of whether this temporal variation in evaporation occurred due to the flare, an unseen associated coronal mass ejection (CME), or even the simultaneous effect of both. In this work, we investigate the impact of flares (radiation), winds, and CMEs (particles) on the atmosphere of HD189733b using three-dimensional radiation hydrodynamic simulations that self-consistently include stellar photon heating. We study four cases: first, the quiescent phase including stellar wind; secondly, a flare; thirdly, a CME; and fourthly, a flare that is followed by a CME. Compared to the quiescent case, we find that the flare alone increases the evaporation rate by only 25 per cent, while the CME leads to a factor of 4 increments. We calculate Ly α synthetic transits and find that the flare alone cannot explain the observed high blueshifted velocities seen in the Ly α. The CME, however, leads to an increase in the velocity of escaping atmospheres, enhancing the blueshifted transit depth. While the effects of CMEs show a promising potential, our models are not able to fully explain the blueshifted transit depths, indicating that they might require additional physical mechanisms.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): planet-star interactions - planets and satellites: atmosphere - stars: HD189733A - stars: coronal mass ejections - stars: flares

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 Ross 905b Pl 11 42 11.0933874353 +26 42 23.658083337           ~ 721 1
2 HD 189733B PM* 20 00 42.9779053104 +22 42 34.178508072       14.67   M4V 16 0
3 HD 189733 BY* 20 00 43.7129433648 +22 42 39.073143456 9.241 8.578 7.648 7.126 6.68 K2V 816 1
4 HD 189733b Pl 20 00 43.7130382888 +22 42 39.071811263           ~ 1293 1
5 HD 209458b Pl 22 03 10.7729598762 +18 53 03.548248479           ~ 1709 1

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2022.10.05-21:26:08

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