Worlds Next Door. III. Indirect Evidence for Enhanced Atmospheric Metallicity and/or the Presence of Water Clouds in the Nearest Jupiter-analog Eri b
arXiv:2602.23423
Abstract
We present the most sensitive direct imaging search for the nearest ( pc) Jupiter-analog exoplanet, Eri b, with JWST/NIRCam coronagraphy between 4-5 m (F444W). We achieve a 5 contrast sensitivity ( mag) in the F444W filter at the expected planet separation of 1". This is the deepest 4-5 m contrast performance achieved for any JWST/NIRCam observation to date at these separations (and better than ground-based limits). Yet, the planet remains elusive to imaging. We update the star's age to Gyr, older than previous age estimates, using the latest gyrochronology relations. This significantly impacts Eri b's inferred effective temperature (), which is now expected to lie between 150-200 K based on evolutionary models for a 1 planet. Using cloud-free Sonora Flame Skimmer models and custom PICASO patchy cloud models in the above range, we find that the F444W non-detection of Eri b can be explained by a metal-enriched atmosphere and/or an atmosphere containing water ice clouds. Both possibilities suggest that Eri b's atmosphere is strikingly similar to that of Jupiter in our Solar System. Alternatively, if we do not enforce the dynamical mass (), a solar metallicity, cloud-free, planet would be consistent with the NIRCam upper limit based on the Sonora Flame Skimmer evolutionary models. Finally, we place limits on the size of a potential ring system using the NIRCam/F210M data and discuss the opportunity to directly image Eri b with additional JWST observations, the Roman Coronagraph Instrument, the ExtraSolar Coronagraph on the Lazuli Observatory, and EELT/METIS.
Accepted to AJ. 27 pages, 14 figures, 5 tables