A Technology and Science Gap List for Habitable-Zone Exoplanet Imaging with Ground-Based Extremely Large Telescopes
Author
Jensen-Clem, R.Hinz, P.
Skemer, A.
Wizinowich, P.
Jovanovic, N.
Mazin, B.A.
Bailey, J.I., III
Frazin, R.A.
Sallum, S.

Males, J.R.
Tamura, M.
Affiliation
University of ArizonaIssue Date
2022-08-29
Metadata
Show full item recordPublisher
SPIECitation
Rebecca Jensen-Clem, Phil Hinz, Andy Skemer, Peter Wizinowich, Nemanja Jovanovic, Benjamin A. Mazin, John I. Bailey III, Richard A. Frazin, Steph Sallum, Jared R. Males, and Motohide Tamura "A technology and science gap list for habitable-zone exoplanet imaging with ground-based extremely large telescopes", Proc. SPIE 12185, Adaptive Optics Systems VIII, 1218503 (29 August 2022); https://doi.org/10.1117/12.2630547Rights
© 2022 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Pathways to Discovery in Astronomy and Astrophysics for the 2020s decadal survey highlighted the ability of the coming generation of 30-meter-class telescopes “to detect, image, and characterize temperate rocky planets around low-mass stars, measure their atmospheric compositions including searches for oxygen.” However, many of the technologies required to reach the challenging contrast ratios associated with this science case are not yet available, and targeted preparatory science must be carried out well in advance of these observations. In this paper, we draw from the example of NASA's Exoplanet Exploration Program and propose a preliminary version of a “Technology Gap List” and “Science Gap List” for the ground-based imaging of rocky planets around the nearest stars with extremely large ground-based telescopes. These lists can be used to prioritize precursor technical demonstrations and observations with current and near-term high contrast instrumentation, so that the community is ready to exploit the collecting area of extremely large telescopes. © 2022 SPIE.Note
Immediate accessISSN
0277-786XVersion
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2630547