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Record W4415352992 · doi:10.1051/0004-6361/202556296

JWST/MIRI observations of the young TWA 27 system: Hydrocarbon disk chemistry, silicate clouds, and evidence of a circumplanetary disk

2025· article· en· W4415352992 on OpenAlexaff
P. Patapis, M. Morales-Calderón, Aditya M. Arabhavi, H. Kühnle, Danny Gasman, Gabriele Cugno, P. Mollière, Elisabeth C. Matthews, Mathilde Mâlin, Niall Whiteford, P. O. Lagage, R. Waters, M. Guêdel, Th. Henning, B. Vandenbussche, O. Absil, I. Argyriou, D. Barrado, P. Baudoz, A. Boccaletti, Jordy Bouwman, Christophe Cossou, A. Coulais, L. Decin, R. Gastaud, A. Glasse, Adrian M. Glauser, Steven L. Grant, M. Min, I. Kamp, G. Olofsson, J. Pye, D. Rouan, P. Royer, S. Scheithauer, Pascal Tremblin, Laura Esther Gangoso de la Colina, T. P. Ray, G. Östlin, E. F. van Dishoeck

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsInstitute of Particle Physics
FundersEuropean Regional Development FundConsejo Superior de Investigaciones CientíficasJet Propulsion LaboratoryAmes Research CenterMax-Planck-Institut für AstronomieKnut och Alice Wallenbergs StiftelseScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeKU LeuvenNederlandse Organisatie voor Wetenschappelijk OnderzoekFonds Wetenschappelijk OnderzoekInstituto Nacional de Técnica AeroespacialEidgenössische Technische Hochschule ZürichChalmers Tekniska HögskolaUtah State UniversityCentre National d’Etudes SpatialesNational Science FoundationBelgian Federal Science Policy OfficeSwedish National Space AgencyFonds De La Recherche Scientifique - FNRSUniversiteit van AmsterdamPaul Scherrer InstitutSpace Telescope Science InstituteUniversiteit LeidenNational Aeronautics and Space AdministrationUniversity College LondonDanmarks GrundforskningsfondNorthrop GrummanCardiff UniversityUniversität zu KölnDublin Institute for Advanced StudiesCalifornia Institute of TechnologyUniversity of BernMinisterio de Ciencia e InnovaciónEuropean CommissionUniversity of LeicesterRijksuniversiteit GroningenAgencia Estatal de InvestigaciónSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNational Research FoundationGoddard Space Flight CenterEuropean Space Agency
KeywordsSpectral lineSilicateAtmosphere (unit)PlanetSpectral energy distributionPhotometry (optics)Emission spectrumPhotosphereSpectrometer

Abstract

fetched live from OpenAlex

Context . The Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST) enables the characterisation of young self-luminous gas giants in a previously inaccessible wavelength range, revealing insights into physical processes of the gas, dust, and clouds. Aims . We aim to characterise the young planetary system TWA 27 (2M1207) in the mid-infrared, revealing the atmosphere and disk spectra of the M9 brown dwarf TWA 27A and its L6 planetary-mass companion TWA 27b. Methods . We obtained data from the MIRI Medium Resolution Spectrometer (MRS) from 4.9 to 20 μm, and MIRI Imaging in the F1000W and F1500W filters. We applied high-contrast imaging data processing methods in order to extract the companion spectral energy distribution up to 15 μm at a separation of 0.″78 and contrast of 60. Using published spectra from JWST/NIRSpec, we analysed the 1-20 μm spectra with self-consistent atmosphere grids, and the molecular disk emission from TWA 27A with 0D slab models. Results . We find that the atmosphere of TWA 27A is well fitted with the BT-SETTL model of effective temperature T eff ~ 2780 K, log g ~ 4.3, and a blackbody component of ∼740 K for the circumstellar disk inner rim. The disk consists of at least 11 organic molecules, and neither water nor silicate dust emission are detected. The atmosphere of the planet TWA 27b matches with a T eff ~ 1400 K low-gravity model when adding extinction, with the ExoREM grid fitting the best. MIRI spectra and photometry for TWA 27b reveal a silicate cloud absorption feature between 8-10 μm, and evidence (>5σ) of infrared excess at 15 μm that is consistent with predictions from circumplanetary disk emission. Conclusions . The MIRI observations present novel insights into the young planetary system TWA 27, showing a diversity of features that can be studied to understand the formation and evolution of circumplanetary disks and young dusty atmospheres.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.012
GPT teacher head0.216
Teacher spread0.204 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations2
Published2025
Admission routes1
Has abstractyes

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