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Record W4399380890 · doi:10.1126/science.adi8147

Abundant hydrocarbons in the disk around a very-low-mass star

2024· article· en· W4399380890 on OpenAlexfundno aff
Aditya M. Arabhavi, I. Kamp, Th. Henning, E. F. van Dishoeck, Valentin Christiaens, Danny Gasman, A. Perrin, M. Güdel, Benoît Tabone, J. S. Kanwar, L. B. F. M. Waters, Ilaria Pascucci, M. Samland, Giulia Perotti, Giulio Bettoni, Sierra L. Grant, Pierre-Olivier Lagage, T. P. Ray, B. Vandenbussche, Olivier Absil, Ioannis Argyriou, D. Barrado, A. Boccaletti, J. Bouwman, A. Caratti o Garatti, Adrian M. Glauser, F. Lahuis, Michael Mueller, G. Olofsson, E. Pantin, Silvia Scheithauer, M. Morales‐Calderón, Riccardo Franceschi, Hyerin Jang, Nicole Pawellek, Donna Rodgers-Lee, J. Schreiber, Kamber R. Schwarz, Milou Temmink, Marissa Vlasblom, Gillian Wright, L. Colina, Göran Östlin

Bibliographic record

VenueScience · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsnot available
FundersHorizon 2020 Framework ProgrammeMinisterio de Ciencia e InnovaciónBelgian Federal Science Policy OfficeCentre National d’Etudes SpatialesVlaamse regeringFonds De La Recherche Scientifique - FNRSSwedish National Space AgencyCanadian Space AgencyScience Foundation IrelandNederlandse Organisatie voor Wetenschappelijk OnderzoekSpace Telescope Science InstituteScience and Technology Facilities CouncilNational Research FoundationAgencia Estatal de InvestigaciónEnterprise IrelandDanmarks GrundforskningsfondEuropean Space AgencyFonds Wetenschappelijk OnderzoekNational Aeronautics and Space Administration
KeywordsPlanetProtoplanetary diskDebris diskAstrophysicsPhysicsStarsAstrobiologyCarbon fibersTerrestrial planetPlanetary systemPlanetary massAstronomyMaterials science

Abstract

fetched live from OpenAlex

Very-low-mass stars (those less than 0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars. The compositions of those planets are largely unknown but are expected to relate to the protoplanetary disk in which they form. We used James Webb Space Telescope mid-infrared spectroscopy to investigate the chemical composition of the planet-forming disk around ISO-ChaI 147, a 0.11-solar-mass star. The inner disk has a carbon-rich chemistry; we identified emission from 13 carbon-bearing molecules, including ethane and benzene. The high column densities of hydrocarbons indicate that the observations probe deep into the disk. The high carbon-to-oxygen ratio indicates radial transport of material within the disk, which we predict would affect the bulk composition of any planets forming in the disk.

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 score0.002
Threshold uncertainty score0.003

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)0.0000.000

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 head0.009
GPT teacher head0.253
Teacher spread0.244 · 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".

Quick stats

Citations60
Published2024
Admission routes1
Has abstractyes

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