A comparison of simulated JWST observations derived from equilibrium and non-equilibrium chemistry models of giant exoplanets
We aim to see if the difference between equilibrium and disequilibrium chemistry is observable in the atmospheres of transiting planets by the James Webb Space Telescope (JWST). We perform a case study comparing the dayside emission spectra of three planets like HD 189733b, WASP-80b, and GJ 436b, in...
| المؤلفون الرئيسيون: | , , , , , , |
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| التنسيق: | Journal article |
| منشور في: |
Institute of Physics
2018
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