TY - JOUR
T1 - Optical calibration and first light for the deformable mirror demonstration mission CubeSat (DeMi)
AU - Morgan, Rachel
AU - Douglas, Ewan
AU - Allan, Gregory
AU - Do Vale Pereira, Paula
AU - Gubner, Jennifer
AU - Haughwout, Christian
AU - Holden, Bobby
AU - Murphy, Thomas
AU - Merk, John
AU - Egan, Mark
AU - Furesz, Gabor
AU - Roascio, Danilo
AU - Xin, Yinzi
AU - Cahoy, Kerri
N1 - Funding Information:
This material is based upon work supported by the Defense Advanced Research Projects Agency (DARPA) Program Office under Contract No. W31P4Q-16-C-0089. The DeMi mission is managed by Aurora Flight Sciences. The DeMi bus was built by Blue Canyon Technologies. DeMi spacecraft environmental testing was conducted at the MIT Lincoln Laboratory Environmental Testing Laboratory. ETL staff including Kelly Beattie, Ron Efromson, Scott Hillis, Jon Howell, and Joseph Orender provided invaluable expertise throughout spacecraft testing. Chris Chesbrough from MIT Lincoln Laboratory was instrumental in helping the DeMi team with bonding of optical components. Nanoracks LLC was the launch provider for the DeMi spacecraft and provided equipment and instruction for spacecraft vibration testing. The MIT Kavli Institute generously provided access to an interferometer and clean room space for DeMi alignment and spacecraft testing. Rachel Morgan is a NASA Space Technology Research Fellow under grant 80NSSC18K1182. Yinzi Xin is a NSF Graduate Research Fellow under grant 1122374. This research made use of POPPY, an open-source optical propagation Python package originally developed for the James Webb Space Telescope.31 This research also made use of Numpy46 and Astropy,47 a community-developed core Python package for astronomy.48 The authors have no known conflicts of interest to declare.
Publisher Copyright:
© The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
PY - 2021/4/1
Y1 - 2021/4/1
N2 - Microelectromechanical systems (MEMS) deformable mirrors (DMs) can provide high-precision wavefront control with a small form-factor, low power device. This makes them a key technology option for future space telescopes requiring adaptive optics for high-contrast imaging of exoplanets with a coronagraph instrument. The Deformable Mirror Demonstration Mission (DeMi) CubeSat payload is a miniature space telescope designed to demonstrate MEMS DM technology in space for the first time. The DeMi payload contains a 50-mm primary mirror, an internal calibration laser source, a 140-actuator MEMS DM from Boston Micromachines Corporation, an image plane wavefront sensor, and a Shack-Hartmann wavefront sensor (SHWFS). The key DeMi payload requirements are to measure individual actuator wavefront displacement contributions to a precision of 12 nm and correct both static and dynamic wavefront errors in space to less than 100-nm RMS error. The DeMi mission will raise the technology readiness level of MEMS DM technology from a five to at least a seven for future space telescope applications. We summarize the DeMi optical payload design, calibration, optical diffraction model, alignment, integration, environmental testing, and preliminary data from in-space operations. Ground testing data show that the DeMi SHWFS can measure individual actuator deflections on the MEMS DM to within 10 nm of interferometric calibration measurements and can meet the 12-nm precision mission requirement for actuator deflection voltages between 0 and 120 V. Payload data from throughout environmental testing show that the MEMS DM and DeMi payload survived environmental testing and provides a valuable baseline to compare with space data. Initial data from space operations show the MEMS DM actuating in space with a median agreement between individual actuator measurements from space and equivalent ground testing data of 12 nm.
AB - Microelectromechanical systems (MEMS) deformable mirrors (DMs) can provide high-precision wavefront control with a small form-factor, low power device. This makes them a key technology option for future space telescopes requiring adaptive optics for high-contrast imaging of exoplanets with a coronagraph instrument. The Deformable Mirror Demonstration Mission (DeMi) CubeSat payload is a miniature space telescope designed to demonstrate MEMS DM technology in space for the first time. The DeMi payload contains a 50-mm primary mirror, an internal calibration laser source, a 140-actuator MEMS DM from Boston Micromachines Corporation, an image plane wavefront sensor, and a Shack-Hartmann wavefront sensor (SHWFS). The key DeMi payload requirements are to measure individual actuator wavefront displacement contributions to a precision of 12 nm and correct both static and dynamic wavefront errors in space to less than 100-nm RMS error. The DeMi mission will raise the technology readiness level of MEMS DM technology from a five to at least a seven for future space telescope applications. We summarize the DeMi optical payload design, calibration, optical diffraction model, alignment, integration, environmental testing, and preliminary data from in-space operations. Ground testing data show that the DeMi SHWFS can measure individual actuator deflections on the MEMS DM to within 10 nm of interferometric calibration measurements and can meet the 12-nm precision mission requirement for actuator deflection voltages between 0 and 120 V. Payload data from throughout environmental testing show that the MEMS DM and DeMi payload survived environmental testing and provides a valuable baseline to compare with space data. Initial data from space operations show the MEMS DM actuating in space with a median agreement between individual actuator measurements from space and equivalent ground testing data of 12 nm.
KW - Adaptive optics
KW - Cubesats
KW - Deformable mirrors
UR - http://www.scopus.com/inward/record.url?scp=85110579689&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85110579689&partnerID=8YFLogxK
U2 - 10.1117/1.JATIS.7.2.024002
DO - 10.1117/1.JATIS.7.2.024002
M3 - Article
AN - SCOPUS:85110579689
VL - 7
JO - Journal of Astronomical Telescopes, Instruments, and Systems
JF - Journal of Astronomical Telescopes, Instruments, and Systems
SN - 2329-4124
IS - 2
M1 - 024002
ER -