Comparative Planetary Atmospheres: Models of TrES-1 and HD209458b

Abstract

We present new self-consistent atmosphere models for transiting planets TrES-1 and HD209458b. The planets were recently observed with the Spitzer Space Telescope in bands centered on 4.5 and 8.0 $μ$m, for TrES-1, and 24 $μ$m, for HD209458b. We find that standard solar metallicity models fit the observations for HD209458b. For TrES-1, which has an T_eff ~300 K cooler, we find that models with a metallicity 3-5 times enhanced over solar abundances can match the 1$σ$ error bar at 4.5 $μ$m and 2$σ$ at 8.0$μ$m. Models with solar abundances that included energy deposition into the stratosphere give fluxes that fall within the 2$σ$ error bars in both bands. The best-fit models for both planets assume that reradiation of absorbed stellar flux occurs over the entire planet. For all models of both planets we predict planet/star flux ratios in other Spitzer bandpasses.