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Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk

  • Authors: William O. Balmer, Laurent Pueyo, Ashley Messier, Evelyn Bruinsma, Jeremy Jones, Klara Matuszewska, Marshall D. Perrin, Julien H. Girard, Jarron M. Leisenring, Kellen Lawson, Roeland P. van der Marel, Jens Kammerer, Aarynn Carter, Mathilde Mâlin, Kimberly Ward-Duong, Kielan K. W. Hoch, Emily Rickman, Sara Seager

William O. Balmer et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 1.

The 4–5 μm color of 29 Cyg b in context. (a) A deconvolved and smoothed three-color composite. Blue is assigned to the F410M filter, green to the F430M filter, and red to the F460M filter, in increasing wavelength; the brightness in each filter is in units of MJy sr–1, normalized to the brightness of the companion in F410M. The location of 29 Cyg A, blocked by the LWBAR/narrow coronagraph, is marked by a cartoon star. (b) Color–color diagram of brown dwarfs and giant planets between 4 and 5 μm. 29 Cyg b exhibits striking similarity with HR 8799 c and e, which are offset toward deeper CO2 absorption from the brown dwarf population. The typical uncertainty for the BDs is 0.03 mag, smaller than the scatter points.

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