Sinking Silicates. I. Characterizing the Benchmark System Containing the T0 Brown Dwarf CWISEJ210640.16+250729.0 using JWST

Abstract In this study, we present the full (97.3% complete) 0.8–12.5 μ m spectral energy distribution (SED) of an L/T transition object, CWISE J210640.16+250729.0 (CW 2106), using the James Webb Space Telescope (JWST). We provide a full characterization of the host star’s elemental abundances and age. We empirically derive the bolometric luminosity (≈ −4.825 dex) of CW 2106, and obtain estimates of its mass ( M ≈ 50–62 M Jup ), radius ( R ≈ 0.83–0.87 R Jup ), effective temperature ( T eff ≈ 1213 K), and surface gravity ( log g ≈ 5.28 dex). We find the near-infrared (near-IR) spectrum (0.8–2.5 μ m) is best reproduced with cloudy atmospheric models while the mid-infrared (mid-IR) spectrum (5–12.5 μ m) is best reproduced with cloudless models. This suggests a cloud layer restricted to only the deepest observable parts of the atmosphere and is qualified by the lack of a 9 μ m silicate feature. Making use of the Mg/Si ratio of the primary, alongside thermochemical models, we predict the clouds in CW 2106 to be composed primarily of enstatite (MgSiO 3 ), removing ∼23% of the bulk oxygen out of the atmosphere. Future retrieval studies will be able to help investigate the existence and full impact of these cloud species.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-10-29
DOI
https://doi.org/10.3847/1538-4357/aea4b2
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Sinking Silicates. I. Characterizing the Benchmark System Containing the T0 Brown Dwarf CWISEJ210640.16+250729.0 using JWST

Jacqueline K. Faherty, Johanna M. Vos, Caprice L. Phillips, Emily Calamari et al.
3 links
The Astrophysical Journal
Stellar, planetary, and galactic studies
article

Sinking Silicates. I. Characterizing the Benchmark System Containing the T0 Brown Dwarf CWISEJ210640.16+250729.0 using JWST

Jacqueline K. Faherty, Johanna M. Vos, Caprice L. Phillips, Emily Calamari, Niall Whiteford, Channon Visscher, Viktória Kecskeméthy, John M. Brewer, Jonathan Gagné, Ben Burningham, Marina E. Gemma, Josefine Gaarn, Genaro Suárez, Austin James Rothermich, Kelle L. Cruz, Catherine Manea, Eileen C. Gonzales, Daniella Carolina Bardalez Gagliuffi, Mark S. Marley
article en

Abstract

Abstract In this study, we present the full (97.3% complete) 0.8–12.5 μ m spectral energy distribution (SED) of an L/T transition object, CWISE J210640.16+250729.0 (CW 2106), using the James Webb Space Telescope (JWST). We provide a full characterization of the host star’s elemental abundances and age. We empirically derive the bolometric luminosity (≈ −4.825 dex) of CW 2106, and obtain estimates of its mass ( M ≈ 50–62 M Jup ), radius ( R ≈ 0.83–0.87 R Jup ), effective temperature ( T eff ≈ 1213 K), and surface gravity ( log g ≈ 5.28 dex). We find the near-infrared (near-IR) spectrum (0.8–2.5 μ m) is best reproduced with cloudy atmospheric models while the mid-infrared (mid-IR) spectrum (5–12.5 μ m) is best reproduced with cloudless models. This suggests a cloud layer restricted to only the deepest observable parts of the atmosphere and is qualified by the lack of a 9 μ m silicate feature. Making use of the Mg/Si ratio of the primary, alongside thermochemical models, we predict the clouds in CW 2106 to be composed primarily of enstatite (MgSiO 3 ), removing ∼23% of the bulk oxygen out of the atmosphere. Future retrieval studies will be able to help investigate the existence and full impact of these cloud species.

The Astrophysical JournalVol. 1011(1)
National Aeronautics and Space Administration, Space Telescope Science Institute
Openalex Percentile: Top 28%
Stellar, planetary, and galactic studies
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