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Protoplanetary Disk Science Enabled by Extremely Large Telescopes

Jang-Condell, Hannah and Brittain, Sean and Weinberger, Alycia and Liu, Michael and Faherty, Jacqueline and Bae, Jaehan and Andrews, Sean and Ansdell, Megan and Birnstiel, Til and Boss, Alan and Close, Laird and Currie, Thayne and Desch, Steven J and Dodson-Robinson, Sarah and Dong, Chuanfei and Duchene, Gaspard and Espaillat, Catherine and Follette, Kate and Gaidos, Eric and Gao, Peter and Haghighipour, Nader and Hartnett, Hilairy and Hasegawa, Yasuhiro and Kama, Mihkel and Kim, Jinyoung Serena and Kóspál, Ágnes and Lisse, Carey and Lyra, Wladimir and Macintosh, Bruce and Mawet, Dimitri and McGehee, Peregrine and Meyer, Michael and Peretz, Eliad and Perez, Laura and Pontoppidan, Klaus and Sallum, Steph and Salyk, Colette and Szentgyorgyi, Andrew and Wagner, Kevin (2019) Protoplanetary Disk Science Enabled by Extremely Large Telescopes. Astro2020 Science White Paper, . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190619-101806526

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Abstract

The processes that transform gas and dust in circumstellar disks into diverse exoplanets remain poorly understood. One key pathway is to study exoplanets as they form in their young (∼few~Myr) natal disks. Extremely Large Telescopes (ELTs) such as GMT, TMT, or ELT, can be used to establish the initial chemical conditions, locations, and timescales of planet formation, via (1)~measuring the physical and chemical conditions in protoplanetary disks using infrared spectroscopy and (2)~studying planet-disk interactions using imaging and spectro-astrometry. Our current knowledge is based on a limited sample of targets, representing the brightest, most extreme cases, and thus almost certainly represents an incomplete understanding. ELTs will play a transformational role in this arena, thanks to the high spatial and spectral resolution data they will deliver. We recommend a key science program to conduct a volume-limited survey of high-resolution spectroscopy and high-contrast imaging of the nearest protoplanetary disks that would result in an unbiased, holistic picture of planet formation as it occurs.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1903.05077arXivDiscussion Paper
ORCID:
AuthorORCID
Mawet, Dimitri0000-0002-8895-4735
Record Number:CaltechAUTHORS:20190619-101806526
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190619-101806526
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96554
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Jun 2019 17:40
Last Modified:19 Jun 2019 17:40

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