The formation and migration history of a planet is expected to be imprinted in its atmosphere, in particular its carbon-to-oxygen (C/O) ratio and metallicity. The BOWIE-ALIGN programme is performing a comparative study of JWST spectra of four aligned and four misaligned hot Jupiters, with the aim of characterising their atmospheres and ...
The formation and migration history of a planet is expected to be imprinted in its atmosphere, in particular its carbon-to-oxygen (C/O) ratio and metallicity. The BOWIE-ALIGN programme is performing a comparative study of JWST spectra of four aligned and four misaligned hot Jupiters, with the aim of characterising their atmospheres and corroborating the link between the observables and the formation history. In this work, we present the 2.8 − 5.2 micron transmission spectrum of TrES-4 b, a hot Jupiter with an orbit aligned with the rotation axis of its F-type host star. Using free chemistry atmospheric retrievals, we report a confident detection of H2O at an abundance of log 𝑋H2O = −2.98+0.68 −0.73 at a significance of 8.4𝜎. We also find evidence for CO and small amounts of CO2, retrieving abundances log 𝑋CO = −3.76+0.89 −1.01 and log 𝑋CO2 = −6.86+0.62 −0.65 (3.1𝜎 and 4.0𝜎 respectively). The observations are consistent with the the atmosphere being in chemical equilibrium; our retrievals yield C/O between 0.30 − 0.42 and constrain the atmospheric metallicity to the range 0.4 − 0.7× solar. The inferred sub-stellar properties (C/O and metallicity) challenge traditional models, and could have arisen from an oxygen-rich gas accretion scenario, or a combination of low-metallicity gas and carbon-poor solid accretion
