A Future Large-Aperture UVOIR Space Observatory: Key Technologies and Capabilities

Bolcar, Matthew Ryan; Stahle, Carl M.; Balasubramaniam, Kunjithapatham; Clampin, Mark; Feinberg, Lee D.; Mosier, Gary E.; Quijada, Manuel A.; Rauscher, Bernard J.; Redding, David C.; Rioux, Norman M.; Shaklan, Stuart B.; Stahl, H. Philip; Thronson, Harley A.

NASA NTRS · 20150000801

A Future Large-Aperture UVOIR Space Observatory: Key Technologies and Capabilities

Bolcar, Matthew Ryan·Stahle, Carl M.·Balasubramaniam, Kunjithapatham·Clampin, Mark·Feinberg, Lee D.·Mosier, Gary E.·Quijada, Manuel A.·Rauscher, Bernard J.·Redding, David C.·Rioux, Norman M.·Shaklan, Stuart B.·Stahl, H. Philip·Thronson, Harley A.

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Abstract

We present the key technologies and capabilities that will enable a future, large-aperture ultravioletopticalinfrared (UVOIR) space observatory. These include starlight suppression systems, vibration isolation and control systems, lightweight mirror segments, detector systems, and mirror coatings. These capabilities will provide major advances over current and near-future observatories for sensitivity, angular resolution, and starlight suppression. The goals adopted in our study for the starlight suppression system are 10-10 contrast with an inner working angle of 20 milliarcsec and broad bandpass. We estimate that a vibration and isolation control system that achieves a total system vibration isolation of 140 dB for a vibration-isolated mass of 5000 kg is required to achieve the high wavefront error stability needed for exoplanet coronagraphy. Technology challenges for lightweight mirror segments include diffraction-limited optical quality and high wavefront error stability as well as low cost, low mass, and rapid fabrication. Key challenges for the detector systems include visible-blind, high quantum efficiency UV arrays, photon counting visible and NIR arrays for coronagraphic spectroscopy and starlight wavefront sensing and control, and detectors with deep full wells with low persistence and radiation tolerance to enable transit imaging and spectroscopy at all wavelengths. Finally, mirror coatings with high reflectivity ( 90), high uniformity ( 1) and low polarization ( 1) that are scalable to large diameter mirror substrates will be essential for ensuring that both high throughput UV observations and high contrast observations can be performed by the same observatory.

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Bolcar, Matthew Ryan, Stahle, Carl M., Balasubramaniam, Kunjithapatham, Clampin, Mark, Feinberg, Lee D., Mosier, Gary E., Quijada, Manuel A., Rauscher, Bernard J., Redding, David C., Rioux, Norman M., Shaklan, Stuart B., Stahl, H. Philip, Thronson, Harley A.. 2015-01-04. A Future Large-Aperture UVOIR Space Observatory: Key Technologies and Capabilities. https://ntrs.nasa.gov/citations/20150000801

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