Poster + Paper
29 August 2022 The Planetary Systems Imager for TMT: driving science cases and top level requirements
Author Affiliations +
Conference Poster
Abstract
The Planetary Systems Imager (PSI) is a second-generation exoplanet detection and characterization instrument concept for the Thirty Meter Telescope (TMT). PSI will enable extreme adaptive optics imaging and spectroscopy from the visible into the infrared. Its high contrast, coupled with TMT’s sensitivity, will access entirely new regions of exoplanet parameter space. Here we describe the driving exoplanet science cases for PSI, including detecting and characterizing rocky planets around nearby M dwarfs, constraining atmospheric and surface compositions and variability, measuring accretion onto protoplanets on Solar System orbital scales, and more. We present the top level instrument requirements for each subsystem, which we derive from these science cases and inform using simulations. We discuss PSI’s expected science outcomes for exoplanet studies, and also highlight examples of its potential for Solar System, galactic, and extragalactic science.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephanie Sallum, Max A. Millar-Blanchaer, Natasha Batalha, Jason Wang, Raquel Martinez, Michael P. Fitzgerald, Andy Skemer, Rebecca Jensen-Clem, Benjamin A. Mazin, Mark Chun, Olivier Guyon, Phil Hinz, Jared Males, and Claire Max "The Planetary Systems Imager for TMT: driving science cases and top level requirements", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 1218446 (29 August 2022); https://doi.org/10.1117/12.2630423
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Planets

Exoplanets

Stars

Adaptive optics

Atmospheric sciences

Solar system

Imaging systems

Back to Top