Presentation
2 October 2024 The Nancy Grace Roman Space Telescope: observatory build, test, and verification status
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Abstract
The Nancy Grace Roman Space Telescope (“Roman”) was prioritized by the 2010 Decadal Survey in Astronomy & Astrophysics and is NASA’s next astrophysics flagship observatory. Launching no earlier than 2026, it will conduct several wide field and time domain surveys, as well as conduct an exoplanet census. Roman’s large field of view, agile survey capabilities, and excellent stability enable these objectives, yet present unique engineering and test challenges. Roman comprises a Spacecraft and the Integrated Payload Assembly (IPA), the latter of which includes the Optical Telescope Assembly (OTA), the primary science Wide Field Instrument, a technology demonstration Coronagraph Instrument, and the Instrument Carrier, which meters the OTA to each instrument. The Spacecraft supports the IPA and includes the Bus, Solar Array Sun Shield, Outer Barrel Assembly, and Deployable Aperture Cover. It provides all required power, attitude control, communications, data storage, and stable thermal control functions as well as shading and straylight protection across the entire field of regard. This paper presents the Observatory as it begins integration and test, as well as describes key test and verification activities.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jeremy S. Perkins, Ed Wollack, Dave Content, Josh Abel, Joanne Baker, Lisa Bartusek, Matthew Bolcar, Bente Eegholm, Lawrence Han, Alexia Harper, Jeff Kruk, Ilya Poberezhskiy, Maxime Rizzo, Josh Schlieder, Scott Smith, Missy Vess, and Neil Zimmerman "The Nancy Grace Roman Space Telescope: observatory build, test, and verification status", Proc. SPIE PC13131, Current Developments in Lens Design and Optical Engineering XXV, PC1313103 (2 October 2024); https://doi.org/10.1117/12.3032499
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