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dc.contributor.authorFortney, Jonathan J.
dc.contributor.authorRobinson, Tyler D.
dc.contributor.authorDomagal-Goldman, Shawn
dc.contributor.authorAmundsen, David Skålid
dc.contributor.authorBrogi, Matteo
dc.contributor.authorClaire, Mark
dc.contributor.authorCrisp, David
dc.contributor.authorHebrard, Eric
dc.contributor.authorImanaka, Hiroshi
dc.contributor.authorKok, Remco de
dc.contributor.authorMarley, Mark S.
dc.contributor.authorTeal, Dillon
dc.contributor.authorBarman, Travis
dc.contributor.authorBernath, Peter
dc.contributor.authorBurrows, Adam
dc.contributor.authorCharbonneau, David
dc.contributor.authorFreedman, Richard S.
dc.contributor.authorGelino, Dawn
dc.contributor.authorHelling, Christiane
dc.contributor.authorHeng, Kevin
dc.contributor.authorJensen, Adam G.
dc.contributor.authorKane, Stephen
dc.contributor.authorKempton, Eliza M. -R.
dc.contributor.authorKopparapu, Ravi Kumar
dc.contributor.authorLewis, Nikole K.
dc.contributor.authorLopez-Morales, Mercedes
dc.contributor.authorLyons, James
dc.contributor.authorLyra, Wladimir
dc.contributor.authorMeadows, Victoria
dc.contributor.authorMoses, Julianne
dc.contributor.authorPierrehumbert, Raymond
dc.contributor.authorVenot, Olivia
dc.contributor.authorWang, Sharon X.
dc.contributor.authorWright, Jason T.
dc.date.accessioned2016-05-11T12:30:04Z
dc.date.available2016-05-11T12:30:04Z
dc.date.issued2016-02-23
dc.identifier.citationFortney , J J , Robinson , T D , Domagal-Goldman , S , Amundsen , D S , Brogi , M , Claire , M , Crisp , D , Hebrard , E , Imanaka , H , Kok , R D , Marley , M S , Teal , D , Barman , T , Bernath , P , Burrows , A , Charbonneau , D , Freedman , R S , Gelino , D , Helling , C , Heng , K , Jensen , A G , Kane , S , Kempton , E M -R , Kopparapu , R K , Lewis , N K , Lopez-Morales , M , Lyons , J , Lyra , W , Meadows , V , Moses , J , Pierrehumbert , R , Venot , O , Wang , S X & Wright , J T 2016 ' The need for laboratory work to aid in the understanding of exoplanetary atmospheres ' Nexus for Exoplanet System Science (NExSS) , pp. 1-18 .en
dc.identifier.otherPURE: 242358064
dc.identifier.otherPURE UUID: 7b6f84b5-99df-4f1f-89fe-37dd3d5d4bfa
dc.identifier.otherArXiv: http://arxiv.org/abs/1602.06305v2
dc.identifier.otherORCID: /0000-0001-9518-089X/work/34103239
dc.identifier.urihttp://hdl.handle.net/10023/8777
dc.description.abstractAdvancements in our understanding of exoplanetary atmospheres, from massive gas giants down to rocky worlds, depend on the constructive challenges between observations and models. We are now on a clear trajectory for improvements in exoplanet observations that will revolutionize our ability to characterize the atmospheric structure, composition, and circulation of these worlds. These improvements stem from significant investments in new missions and facilities, such as JWST and the several planned ground-based extremely large telescopes. However, while exoplanet science currently has a wide range of sophisticated models that can be applied to the tide of forthcoming observations, the trajectory for preparing these models for the upcoming observational challenges is unclear. Thus, our ability to maximize the insights gained from the next generation of observatories is not certain. In many cases, uncertainties in a path towards model advancement stems from insufficiencies in the laboratory data that serve as critical inputs to atmospheric physical and chemical tools. We outline a number of areas where laboratory or ab initio investigations could fill critical gaps in our ability to model exoplanet atmospheric opacities, clouds, and chemistry. Specifically highlighted are needs for: (1) molecular opacity linelists with parameters for a diversity of broadening gases, (2) extended databases for collision-induced absorption and dimer opacities, (3) high spectral resolution opacity data for relevant molecular species, (4) laboratory studies of haze and condensate formation and optical properties, (5) significantly expanded databases of chemical reaction rates, and (6) measurements of gas photo-absorption cross sections at high temperatures. We hope that by meeting these needs, we can make the next two decades of exoplanet science as productive and insightful as the previous two decades.
dc.format.extent18
dc.language.isoeng
dc.publisherNexus for Exoplanet System Science (NExSS)
dc.relation.ispartofen
dc.rights© 2016, The Author(s). This is the final published version of the work, which was originally published at http://arxiv.org/abs/1602.06305en
dc.subjectQB Astronomyen
dc.subject.lccQBen
dc.titleThe need for laboratory work to aid in the understanding of exoplanetary atmospheresen
dc.typeWorking or discussion paperen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.Earth and Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews.St Andrews Isotope Geochemistryen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.urlhttp://arxiv.org/abs/1602.06305en
dc.identifier.urlhttps://nexss.info/en


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