Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy
Recent spectroscopic observations of transiting hot Jupiters have permitted the derivation of the thermal structure and molecular abundances of H 2O, CO 2, CO and CH 4 in these extreme atmospheres. Here, for the first time, we apply the technique of optimal estimation to determine the thermal struct...
| Principais autores: | , , |
|---|---|
| Formato: | Journal article |
| Idioma: | English |
| Publicado em: |
2012
|
| _version_ | 1826281498732396544 |
|---|---|
| author | Lee, J Fletcher, L Irwin, P |
| author_facet | Lee, J Fletcher, L Irwin, P |
| author_sort | Lee, J |
| collection | OXFORD |
| description | Recent spectroscopic observations of transiting hot Jupiters have permitted the derivation of the thermal structure and molecular abundances of H 2O, CO 2, CO and CH 4 in these extreme atmospheres. Here, for the first time, we apply the technique of optimal estimation to determine the thermal structure and composition of an exoplanet by solving the inverse problem. The development of a suite of radiative transfer and retrieval tools for exoplanet atmospheres is described, building upon a retrieval algorithm which is extensively used in the study of our own Solar system. First, we discuss the plausibility of detection of different molecules in the dayside atmosphere of HD189733b and the best-fitting spectrum retrieved from all publicly available sets of secondary eclipse observations between 1.45 and 24μm. Additionally, we use contribution functions to assess the vertical sensitivity of the emission spectrum to temperatures and molecular composition. Over the altitudes probed by the contribution functions, the retrieved thermal structure shows an isothermal upper atmosphere overlying a deeper adiabatic layer (temperature decreasing with altitude), which is consistent with previously reported dynamical and observational results. The formal uncertainties on retrieved parameters are estimated conservatively using an analysis of the cross-correlation functions and the degeneracy between different atmospheric properties. The formal solution of the inverse problem suggests that the uncertainties on retrieved parameters are larger than suggested in previous studies, and that the presence of CO and CH 4 is only marginally supported by the available data. Nevertheless, by including as broad a wavelength range as possible in the retrieval, we demonstrate that available spectra of HD189733b can constrain a family of potential solutions for the atmospheric structure. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS. |
| first_indexed | 2024-03-07T00:29:43Z |
| format | Journal article |
| id | oxford-uuid:7f58b740-bcc1-4e44-9351-d9d0245d9e6c |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T00:29:43Z |
| publishDate | 2012 |
| record_format | dspace |
| spelling | oxford-uuid:7f58b740-bcc1-4e44-9351-d9d0245d9e6c2022-03-26T21:16:24ZOptimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopyJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7f58b740-bcc1-4e44-9351-d9d0245d9e6cEnglishSymplectic Elements at Oxford2012Lee, JFletcher, LIrwin, PRecent spectroscopic observations of transiting hot Jupiters have permitted the derivation of the thermal structure and molecular abundances of H 2O, CO 2, CO and CH 4 in these extreme atmospheres. Here, for the first time, we apply the technique of optimal estimation to determine the thermal structure and composition of an exoplanet by solving the inverse problem. The development of a suite of radiative transfer and retrieval tools for exoplanet atmospheres is described, building upon a retrieval algorithm which is extensively used in the study of our own Solar system. First, we discuss the plausibility of detection of different molecules in the dayside atmosphere of HD189733b and the best-fitting spectrum retrieved from all publicly available sets of secondary eclipse observations between 1.45 and 24μm. Additionally, we use contribution functions to assess the vertical sensitivity of the emission spectrum to temperatures and molecular composition. Over the altitudes probed by the contribution functions, the retrieved thermal structure shows an isothermal upper atmosphere overlying a deeper adiabatic layer (temperature decreasing with altitude), which is consistent with previously reported dynamical and observational results. The formal uncertainties on retrieved parameters are estimated conservatively using an analysis of the cross-correlation functions and the degeneracy between different atmospheric properties. The formal solution of the inverse problem suggests that the uncertainties on retrieved parameters are larger than suggested in previous studies, and that the presence of CO and CH 4 is only marginally supported by the available data. Nevertheless, by including as broad a wavelength range as possible in the retrieval, we demonstrate that available spectra of HD189733b can constrain a family of potential solutions for the atmospheric structure. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS. |
| spellingShingle | Lee, J Fletcher, L Irwin, P Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title | Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title_full | Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title_fullStr | Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title_full_unstemmed | Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title_short | Optimal estimation retrievals of the atmospheric structure and composition of HD189733b from secondary eclipse spectroscopy |
| title_sort | optimal estimation retrievals of the atmospheric structure and composition of hd189733b from secondary eclipse spectroscopy |
| work_keys_str_mv | AT leej optimalestimationretrievalsoftheatmosphericstructureandcompositionofhd189733bfromsecondaryeclipsespectroscopy AT fletcherl optimalestimationretrievalsoftheatmosphericstructureandcompositionofhd189733bfromsecondaryeclipsespectroscopy AT irwinp optimalestimationretrievalsoftheatmosphericstructureandcompositionofhd189733bfromsecondaryeclipsespectroscopy |