# MOVES – IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b

@inproceedings{Barth2021MOVESI,
title={MOVES – IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b},
author={P Barth and Ch. Helling and Eva E. St{\"u}eken and Vincent Bourrier and Nathan J. Mayne and Paul B. Rimmer and M M Jardine and Aline A. Vidotto and Peter J. Wheatley and R Fares},
year={2021}
}
• Published 22 December 2020
• Physics, Geology
Hot Jupiters provide valuable natural laboratories for studying potential contributions of highenergy radiation to prebiotic synthesis in the atmospheres of exoplanets. In this fourth paper of the MOVES (Multiwavelength Observations of an eVaporating Exoplanet and its Star) programme, we study the effect of different types of high-energy radiation on the production of organic and prebiotic molecules in the atmosphere of the hot Jupiter HD 189733b. Our model combines X-ray and UV observations…
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