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  A project in the UMass Lowell, The Planet Imaging
                      Coronagraphic Technology Using a Reconfigurable
                      Experimental Base mission (PICTURE-B) is a NASA
                      sounding rocket mission to directly measure
                      optical light scattered by the debris disk around
                      Epsilon-Eri, a nearby K2V-type star, 3.2 parsecs
                      (10.5 light years) from Earth, with the relatively
                      young age of approximately 1 billion years. 
    PICTURE-B consists of a 0.5 meter telescope and
                      visible nulling coronograph instrument (a
                      "nuller") to attenuate the overwhelmingly bright
                      light from a star, while enabling dim light from
                      material around the star to reach the science
                      camera. The electronics section on PICTURE-B
                      includes three networked computers, controlling
                      the nuller, the science and wavefront sensing
                      cameras and the fine pointing system. In the
                      future, PICTURE-B can be reconfigured for extended
                      balloon born observations of fainter, more
                      distant, debris disks.  
     While PICTURE-B's scientific objectives are
                      spectacular, its technology objectives are equally
                      important impact. By demonstrating a visible
                      nulling coronograph and a deformable mirror in the
                      space environment, PICTURE-B will significantly
                      advance the broader goal of direct imaging of
                      Earth-like planets.  The PICTURE-B nuller was previously launched on a
                      NASA sounding rocket from White Sands Missile
                      Range in Oct. 2011 as the PICTURE mission,
                      successfully demonstrating flight-worthiness and
                      the fine steering technology. The remarkable fine
                      steering control, required by the PICTURE-B
                      mission and future missions to image exoplanets,
                      kept the telescope pointed at the star Rigel to
                      within a few millions of a degree (see 
                        Mendillo et al. 2012a ). Unfortunately, the
                      science telemetry channel failed in-flight and no
                      science data was received. The payload was
                      successfully recovered and the ultra-low-expansion
                      glass primary mirror did not survive re-entry and
                      landing. The PICTURE-B payload will re-fly the
                      original PICTURE nuller and fine steering system,
                      while incorporating a new silicon carbide primary
                      mirror. For a more detailed description of the
                      PICTURE payload, see Mendillo et al 2012, "PICTURE:
                        a Sounding Rocket Experiment for Direct Imaging
                        of an Extrasolar Planetary Environment."  
                      
                        
                          | Team Members:Boston University: 
                            
                            Northrop Grumman Inc: 
                            
			    
                              NASA Goddard Space Flight Center:UMass Lowell:
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  PICTURE-B related publications:
 
 
                       C. B. Mendillo, B. A. Hicks, T. A. Cook, T.
                        G. Bifano, D. A. Content, B. F. Lane, B. M.
                        Levine, D. Rabin, S. R. Rao, R. Samuele, E.
                        Schmidtlin, M. Shao, J. K. Wallace, S.
                        Chakrabarti, 2012. "PICTURE:
                          a Sounding Rocket Experiment for Direct
                          Imaging of an Extrasolar Planetary
                          Environment." Proc. SPIE (September 21).
  C. B. Mendillo, S. Chakrabarti, T. A. Cook,
                        B. A. Hicks, and B. F. Lane, 2012, "Flight
                          demonstration of a milliarcsecond pointing
                          system for direct exoplanet imaging,"
                        Appl. Opt. 51, 7069-7079
 S. R. Rao, J. K. Wallace, R. Samuele, S.
                        Chakrabarti, T. A. Cook, B. A. Hicks, P. G.
                        Jung, B. F. Lane, B. M. Levine, C. B. Mendillo,
                        E. Schmidtlin, M. Shao, and J. B. Stewart, 2008,
                        "Path
                          length control in a nulling coronagraph with a
                          MEMS deformable mirror and a calibration
                          interferometer," Proc. SPIE 6888.
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