Spatially resolving the chemical composition of the planet building blocks Article Swipe
YOU?
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· 2020
· Open Access
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· DOI: https://doi.org/10.1093/mnras/staa2137
The inner regions of protoplanetary discs (from ∼0.1 to 10 au) are the expected birthplace of planets, especially telluric. In those high-temperature regions, solids can experience cyclical annealing, vapourisation, and recondensation. Hot and warm dusty grains emit mostly in the infrared domain, notably in N-band (8–13 μm). Studying their fine chemistry through mid-infrared spectro-interferometry with the new Very Large Telescope Interferometer (VLTI) instrument Multi AperTure mid-Infrared SpectroScopic Experiment (MATISSE), which can spatially resolve these regions, requires detailed dust chemistry models. Using radiative transfer, we derived infrared spectra of a fiducial static protoplanetary disc model with different inner-disc (<1 au) dust compositions. The latter were derived from condensation sequences computed at local thermodynamic equilibrium (LTE) for three initial C/O ratios: subsolar (C/O = 0.4), solar (C/O = 0.54), and supersolar (C/O = 1). The three scenarios return very different N-band spectra, especially when considering the presence of sub-micron-sized dust grains. MATISSE should be able to detect these differences and trace the associated sub-au-scale radial changes. We propose a first interpretation of N-band ‘inner-disc’ spectra obtained with the former VLTI instrument MID-infrared Interferometric instrument (MIDI) on three Herbig stars (HD 142527, HD 144432, HD 163296) and one T Tauri star (AS 209). Notably, we could associate a supersolar (‘carbon-rich’) composition for HD 142527 and a subsolar (‘oxygen-rich’) one for HD 1444432. We show that the inner-disc mineralogy can be very specific and not related to the dust composition derived from spatially unresolved mid-infrared spectroscopy. We highlight the need for including more complex chemistry when interpreting solid-state spectroscopic observations of the inner regions of discs, and for considering dynamical aspects for future studies.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/staa2137
- OA Status
- green
- Cited By
- 4
- References
- 94
- Related Works
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W3043147332Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/staa2137Digital Object Identifier
- Title
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Spatially resolving the chemical composition of the planet building blocksWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2020Year of publication
- Publication date
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2020-07-27Full publication date if available
- Authors
-
A. Matter, F. C. Pignatale, B. LópezList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/staa2137Publisher landing page
- Open access
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YesWhether a free full text is available
- OA status
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greenOpen access status per OpenAlex
- OA URL
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https://arxiv.org/pdf/2007.09385Direct OA link when available
- Concepts
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Physics, Astrophysics, Radiative transfer, Planet, Spectral line, Infrared, Chemical composition, Atmospheric radiative transfer codes, Stars, Accretion (finance), Astronomy, Optics, ThermodynamicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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4Total citation count in OpenAlex
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2025: 1, 2023: 1, 2022: 1, 2021: 1Per-year citation counts (last 5 years)
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94Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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