Probing The Gas That Builds Planets: Results From The JWST MINDS Program
Infrared observations with JWST open up a new window into the chemical composition of the gas in the inner disk (<few au) where planets are built.
Results from the MIRI GTO program MINDS (PI: Th. Henning, co-PI: I. Kamp) are presented for several disks around T Tauri and lower-mass stars. A large diversity in spectra is found. Some disks are very rich in H2O lines whereas other disks show prominent CO2.
The spectra of disks around very low-mass stars (<0.3 MSun, late-M type stars like Trappist-1) are dominated by C2H2 and other hydrocarbon features including those of benzene, suggesting volatile C/O>1.
Together these data point to a rich chemistry in the inner regions that is linked to the physical structure of these disks (e.g., dust traps) and that may be affected by processes such as radial drift of icy pebbles from the outer to the inner disk.
E.F. van Dishoeck, the MINDS team
Comments: 6 pages, 2 figures. To appear in the proceedings of IAU Symposium 393, Planetary Science and Exoplanets in the era of JWST, Z. Benkhaldoun, A. Szentgyorgyi, Y. Moulane, eds. (Cambridge University Press)
Subjects: Astrophysics of Galaxies (astro-ph.GA); Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2412.07853 [astro-ph.GA] (or arXiv:2412.07853v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2412.07853
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Submission history
From: Ewine F. van Dishoeck
[v1] Tue, 10 Dec 2024 19:01:14 UTC (465 KB)
https://arxiv.org/abs/2412.07853
Astrobiology
