Payload characterization for CubeSat demonstration of MEMS deformable mirrors

Coronagraphic space telescopes require wavefront control systems for high-contrast imaging applications such as exoplanet direct imaging. High-actuator-count MEMS deformable mirrors (DM) are a key element of these wavefront control systems yet have not been flown in space long enough to characterize their on-orbit performance. The MEMS Deformable Mirror CubeSat Testbed is a conceptual nanosatellite demonstration of MEMS DM and wavefront sensing technology. The testbed platform is a 3U CubeSat bus. Of the 10 x 10 x 34.05 cm (3U) available volume, a 10 x 10 x 15 cm space is reserved for the optical payload. The main purpose of the payload is to characterize and calibrate the onorbit performance of a MEMS deformable mirror over an extended period of time (months). Its design incorporates both a Shack Hartmann wavefront sensor (internal laser illumination), and a focal plane sensor (used with an external aperture to image bright stars). We baseline a 32-actuator Boston Micromachines Mini deformable mirror for this mission, though the design is flexible and can be applied to mirrors from other vendors. We present the mission design and payload architecture and discuss experiment design, requirements, and performance simulations.

[1]  Karl R. Stapelfeldt,et al.  Extrasolar planets and star formation: science opportunities for future ELTs , 2005, Proceedings of the International Astronomical Union.

[2]  Li Yao,et al.  Novel hierarchically dimensioned deformable mirrors with integrated ASIC driver electronics , 2012, Photonics West - Micro and Nano Fabricated Electromechanical and Optical Components.

[3]  Olivier Guyon,et al.  EXCEDE technology development I: first demonstrations of high contrast at 1.2 λ/D for an Explorer space telescope mission , 2012, Other Conferences.

[4]  Henry R. Hertzfeld,et al.  Cubesats: Cost-effective science and technology platforms for emerging and developing nations , 2011 .

[5]  Robert K. Tyson Principles of Adaptive Optics , 1991 .

[6]  J. E. Kim,et al.  A New Type of Space Telescope for Observation of Extreme Lightning Phenomena in the Upper Atmosphere , 2012, IEEE Transactions on Geoscience and Remote Sensing.

[7]  Olivier Guyon,et al.  The EXoplanetary Circumstellar Environments and Disk Explorer (EXCEDE) , 2012, Other Conferences.

[8]  Bruce A. Macintosh,et al.  Speckle Decorrelation and Dynamic Range in Speckle Noise-limited Imaging , 2002 .

[9]  David Krejci,et al.  A survey and assessment of the capabilities of Cubesats for Earth observation , 2012 .

[10]  Bruce A. Macintosh,et al.  The Gemini Planet Imager: from science to design to construction , 2008, Astronomical Telescopes + Instrumentation.

[11]  K. Cahoy,et al.  Ad hoc CubeSat constellations: Secondary launch coverage and distribution , 2013, 2013 IEEE Aerospace Conference.

[12]  Benjamin F. Lane,et al.  PICTURE: a sounding rocket experiment for direct imaging of an extrasolar planetary environment , 2012, Other Conferences.

[13]  Sara Seager,et al.  Achieving high-precision pointing on ExoplanetSat: initial feasibility analysis , 2010, Astronomical Telescopes + Instrumentation.

[14]  Ben R. Oppenheimer,et al.  High-Contrast Observations in Optical and Infrared Astronomy , 2009 .

[15]  J. Goodman Introduction to Fourier optics , 1969 .

[16]  J. Hardy,et al.  Adaptive Optics for Astronomical Telescopes , 1998 .

[17]  M. Jhabvala,et al.  Programmable microshutter arrays for the JWST NIRSpec: optical performance , 2004, IEEE Journal of Selected Topics in Quantum Electronics.

[18]  K. Cahoy,et al.  Nanosatellites for earth environmental monitoring: The MicroMAS project , 2012, 2012 12th Specialist Meeting on Microwave Radiometry and Remote Sensing of the Environment (MicroRad).

[19]  J. Angel,et al.  Ground-based imaging of extrasolar planets using adaptive optics , 1994, Nature.

[20]  James Cutler,et al.  The attitude determination system of the RAX satellite , 2012 .

[21]  Pascal Lorenz,et al.  A survey of small satellites domain: challenges, applications and communications key issues , 2010, SocInfo 2010.

[22]  Olivier Guyon,et al.  ACCESS -- A Science and Engineering Assessment of Space Coronagraph Concepts for the Direct Imaging and Spectroscopy of Exoplanetary Systems , 2009 .

[23]  Erkin Sidick,et al.  Broadband performance of TPF's high-contrast imaging testbed: modeling and simulations , 2006, SPIE Optics + Photonics.

[24]  Russell B. Makidon,et al.  The Structure of High Strehl Ratio Point-Spread Functions , 2003 .

[25]  Jordi Puig-Suari,et al.  CubeSat: A New Generation of Picosatellite for Education and Industry Low-Cost Space Experimentation , 2000 .

[26]  Sug-Whan Kim,et al.  MEMS micromirror characterization in space environments. , 2009, Optics express.

[27]  S. Ridgway,et al.  Exoplanet Imaging with a Phase-induced Amplitude Apodization Coronagraph. I. Principle , 2004, astro-ph/0412179.