Optical alignment of contamination-sensitive far-ultraviolet spectrographs for Aspera SmallSat mission

Aspera is a NASA Astrophysics Pioneers SmallSat mission designed to study diffuse Ovi emission from the warm-hot phase gas in the halos of nearby galaxies. Its payload consists of two identical Rowland Circle-type long-slit spectrographs, sharing a single MicroChannel plate detector. Each spectrograph channel consists of an off-axis parabola primary mirror and a toroidal diffraction grating optimized for the 1013-1057 Å bandpass. Despite the simple configuration, the optical alignment/integration process for Aspera is challenging due to tight optical alignment tolerances, driven by the compact form factor, and the contamination sensitivity of the Far-Ultraviolet optics and detectors. In this paper, we discuss implementing a novel multi-phase approach to meet these requirements using state-of-the-art optical metrology tools. For coarsely positioning the optics we use a blue-laser 3D scanner while the fine alignment is done with a Zygo interferometer and a custom computer-generated hologram. The detector focus requires iterative in-vacuum alignment using a Vacuum UV collimator. The alignment is done in a controlled cleanroom facility at the University of Arizona.

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Published
2024-08-21
DOI
https://doi.org/10.1117/12.3020822
Primary Topic
Spacecraft Design and Technology
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article
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article

Optical alignment of contamination-sensitive far-ultraviolet spectrographs for Aspera SmallSat mission

Daniel Truong, Jacob R. Chambers, Sooseong Park, Dennis Zaritsky et al.
Spacecraft Design and Technology
article

Optical alignment of contamination-sensitive far-ultraviolet spectrographs for Aspera SmallSat mission

Daniel Truong, Jacob R. Chambers, Sooseong Park, Dennis Zaritsky, Aafaque R. Khan, Peter Behroozi, Thomas J. McMahon, Haeun Chung, John Kidd, Lauren Corlies, Heejoo Choi, Rebecca Su, Trenton Brendel, Jamison Noenickx, Keri Hoadley, Walter M. Harris, Ewan S. Douglas, Carlos J. Vargas, Harrison Bradley, Oswald H. W. Siegmund, Hannah Tanquary, D. Hamara, J. Christopher Howk, Daewook Kim, C. W. Hergenrother, Ellie Wolcott, Fernando Coronado, Erika Hamden, Ramona Augustin, Simran Agarwal, Jason Corliss, M. Keppler, Nicole Melso, Sumedha Uppnor, Giulia Ghidoli, Naomi Yescas, Bill Verts, Jacob Vider, Jessica Li, Elijah Garcia, Ipek Nazende Kerkeser, Sanford Selznic, Ralf-J ̈urgen Dettmar, David Schiminovich, Ryan Pecha, Gabe Noriega, Joe Burchett, Jasmine Martinez Castillo, Cork Sauve, A. W. Goodwin, Greyson Davis
article en

Abstract

Aspera is a NASA Astrophysics Pioneers SmallSat mission designed to study diffuse Ovi emission from the warm-hot phase gas in the halos of nearby galaxies. Its payload consists of two identical Rowland Circle-type long-slit spectrographs, sharing a single MicroChannel plate detector. Each spectrograph channel consists of an off-axis parabola primary mirror and a toroidal diffraction grating optimized for the 1013-1057 Å bandpass. Despite the simple configuration, the optical alignment/integration process for Aspera is challenging due to tight optical alignment tolerances, driven by the compact form factor, and the contamination sensitivity of the Far-Ultraviolet optics and detectors. In this paper, we discuss implementing a novel multi-phase approach to meet these requirements using state-of-the-art optical metrology tools. For coarsely positioning the optics we use a blue-laser 3D scanner while the fine alignment is done with a Zygo interferometer and a custom computer-generated hologram. The detector focus requires iterative in-vacuum alignment using a Vacuum UV collimator. The alignment is done in a controlled cleanroom facility at the University of Arizona.

Vol. 363
New Mexico State University (US), University of Iowa (US), Space Telescope Science Institute (US), Adler Planetarium (US), University of Arizona (US), Lunar and Planetary Institute (US), Ruhr University Bochum (DE)
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Spacecraft Design and Technology
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