Exo-C: a probe-scale space mission to directly image and spectroscopically characterize exoplanetary systems using an internal coronagraph

• Main Authors: Stapelfeldt, Karl R. (Author), Brenner, Michael P. (Author), Warfield, Keith R. (Author), Dekens, Frank G. (Author), Belikov, Ruslan (Author), Brugarolas, Paul B. (Author), Bryden, Geoffrey (Author), Chakrabarti, Supriya (Author), Dubovitsky, Serge (Author), Effinger, Robert T. (Author), Hirsch, Brian (Author), Kissil, Andrew (Author), Krist, John E. (Author), Lang, Jared J. (Author), Marley, Mark S. (Author), McElwain, Michael W. (Author), Meadows, Victoria S. (Author), Nissen, Joel (Author), Oseas, Jeffrey M. (Author), Serabyn, Eugene (Author), Sunada, Eric (Author), Trauger, John T. (Author), Unwin, Stephen C. (Author), Cahoy, Kerri (Contributor)
• Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics (Contributor)
• Format: Article
• Language: English
• Published: SPIE, 2018-05-11T20:09:58Z.
• Subjects: Article
• Online Access: Get fulltext

 "Exo-C" is NASA's first community study of a modest aperture space telescope designed for high contrast observations of exoplanetary systems. The mission will be capable of taking optical spectra of nearby exoplanets in reflected light, discover previously undetected planets, and imaging structure in a large sample of circumstellar disks. It will obtain unique science results on planets down to super-Earth sizes and serve as a technology pathfinder toward an eventual flagship-class mission to find and characterize habitable exoplanets. We present the mission/payload design and highlight steps to reduce mission cost/risk relative to previous mission concepts. At the study conclusion in 2015, NASA will evaluate it for potential development at the end of this decade.