The dry and carbon poor inner disk of TW Hya: evidence for a massive icy dust trap
arXiv:1911.11152 · doi:10.1051/0004-6361/201936638
Abstract
Gas giants accrete their envelopes from the gas and dust of proto-planetary disks, so it is important to determine the composition of the inner few AU, where most giant planets are expected to form. We aim to constrain the elemental carbon and oxygen abundance in the inner disk (2.3 AU) of TW Hya and compare with the outer disk ( AU) where carbon and oxygen appear underabundant by a factor of 50. Archival infrared observations of TW Hya are compared with a detailed thermo-chemical model, DALI. The inner disk gas mass and elemental C and O abundances are varied to fit the infrared CO, H and HO line fluxes. Best fitting models have an inner disk that has a gas mass of with C/H and O/H . The elemental oxygen and carbon abundances of the inner disk are times underabundant compared to the ISM and are consistent with those found in the outer disk. The uniformly low volatile abundances imply that the inner disk is not enriched by ices on drifting bodies that evaporate. This indicates that drifting grains are stopped in a dust trap outside the water ice line. Such a dust trap would also form a cavity as seen in high resolution sub-millimeter continuum observations. If CO is the major carbon carrier in the ices, dust needs to be trapped efficiently outside the CO ice line of 20 AU. This would imply that the shallow sub-millimeter rings in the TW Hya disk outside of 20 AU correspond to very efficient dust traps. The more likely scenario is that more than 98\% of the CO has been converted into less volatile species, e.g. CO and CHOH. A giant planet forming in the inner disk would be accreting gas with low carbon and oxygen abundances as well as very little icy dust, potentially leading to a planet atmosphere with strongly substellar C/H and O/H ratios.
arXiv comment6 pages, 3 figures, accepted to A&A letters
References in corpus (43)
- An atomic and molecular database for analysis of submillimetre line observations
- Origins of Hot Jupiters
- The Spitzer ice legacy: Ice evolution from cores to protostars
- Ringed Substructure and a Gap at 1 AU in the Nearest Protoplanetary Disk
- Planet formation around stars of various masses: The snow line and the frequency of giant planets
- Rotational quenching of CO due to H collisions
- An Old Disk That Can Still Form a Planetary System
- The Definitive Abundance of Interstellar Oxygen
- Detection of the Water Reservoir in a Forming Planetary System
- The TW Hya Disk at 870 microns: Comparison of CO and Dust Radial Structures
- The warm gas atmosphere of the HD 100546 disk seen by Herschel (Evidence of a gas-rich, carbon-poor atmosphere?)
- Spectro-astrometric imaging of molecular gas within protoplanetary disk gaps
- Chemical enrichment of giant planets and discs due to pebble drift
- Survival of molecular gas in cavities of transition disks (I. CO)
- The Radial Distribution of H2 and CO in TW Hya as Revealed by Resolved ALMA Observations of CO Isotopologues
- A Spitzer Survey of Mid-Infrared Molecular Emission from Protoplanetary Disks II: Correlations and LTE Models
- The molecular composition of the planet-forming regions of protoplanetary disks across the luminosity regime
- Volatile carbon locking and release in protoplanetary disks. A study of TW Hya and HD 100546
- Lupus disks with faint CO isotopologues: low gas/dust or large carbon depletion?
- A Significantly Low CO Abundance Toward the TW Hya Protoplanetary Disk: A Path to Active Carbon Chemistry?
- Setting the volatile composition of (exo)planet-building material. Does chemical evolution in disk midplanes matter?
- Mass inventory of the giant-planet formation zone in a solar nebula analog
- Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift
- CO destruction in protoplanetary disk midplanes: inside versus outside the CO snow surface
- On the structure of the transition disk around TW Hya
- Evidence for a Snow Line Beyond the Transitional Radius in the TW Hya Protoplanetary Disk
- Emission Lines from the Gas Disk around TW Hydra and the Origin of the Inner Hole
- Unlocking CO Depletion in Protoplanetary Disks I. The Warm Molecular Layer
- Spitzer Spectroscopy of the Transition Object TW Hya
- Tracing water vapor and ice during dust growth
- HD far infrared emission as a measure of protoplanetary disk mass
- The depletion of water during dispersal of planet-forming disk regions
- Survey of cold water lines in protoplanetary disks: indications of systematic volatile depletion
- Ex Lupi from Quiescence to Outburst: Exploring the LTE Approach in Modelling Blended H2O and OH Mid-Infrared Emission
- CO2 infrared emission as a diagnostic of planet-forming regions of disks
- Ro-vibrational excitation of an organic molecule (HCN) in protoplanetary disks
- Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks
- The chemistry of disks around T Tauri and Herbig Ae/Be stars
- Efficiency of radial transport of ices in protoplanetary disks probed with infrared observations: the case of CO
- New Parallaxes and a Convergence Analysis for the TW Hya Association
- H2, CO, and Dust Absorption through Cold Molecular Clouds
- Probing planet formation and disk substructures in the inner disk of Herbig Ae stars with CO rovibrational emission
- Quantum Calculation of Inelastic CO Collisions with H. III. Rate Coefficients for Ro-vibrational Transitions
Cited by in corpus (17)
- Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy
- CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing
- The diverse chemistry of protoplanetary disks as revealed by JWST
- Transition disks: the observational revolution from SEDs to imaging
- Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition
- Forming pressure-traps at the snow-line to isolate isotopic reservoirs in the absence of a planet
- Tracing pebble drift and trapping using radial carbon depletion profiles in protoplanetary disks
- Measuring the atomic composition of planetary building blocks
- If you like C/O variations, you should have put a ring on it
- High Spatial Resolution Observations of Molecular Lines towards the Protoplanetary Disk around TW Hya with ALMA
- Investigating the asymmetric chemistry in the disk around the young star HD 142527
- Discovery of Line Pressure Broadening and Direct Constraint on Gas Surface Density in a Protoplanetary Disk
- No Significant Correlation between Line-emission and Continuum Substructures in the Molecules with ALMA at Planet-forming Scales Program
- Modeling Nitrogen Fractionation in the Protoplanetary Disk around TW Hya: Model Constraints on Grain Population and Carbon-to-Oxygen Elemental Abundance Ratio
- The cosmochemistry of planetary systems
- First Detection of HC5N in a Class II Disk around TW Hya
- Water UV-shielding in the terrestrial planet-forming zone: Implications from water emission