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Proceedings Paper

The Stellar Imager (SI) vision mission
Author(s): Kenneth G. Carpenter; Carolus J. Schrijver; Margarita Karovska
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Paper Abstract

The Stellar Imager (SI) is a UV-Optical, Space-Based Interferometer designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and of the Universe in general and asteroseismic imaging of stellar interiors. SI is identified as a "Flagship and Landmark Discovery Mission" in the 2005 Sun Solar System Connection (SSSC) Roadmap and as a candidate for a "Pathways to Life Observatory" in the Exploration of the Universe Division (EUD) Roadmap (May, 2005). SI will revolutionize our view of many dynamic astrophysical processes: its resolution will transform point sources into extended sources, and snapshots into evolving views. SI's science focuses on the role of magnetism in the Universe, particularly on magnetic activity on the surfaces of stars like the Sun. SI's prime goal is to enable long-term forecasting of solar activity and the space weather that it drives. SI will also revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. The results of the SI "Vision Mission" Study are presented in this paper. Additional information on the SI mission concept and related technology development can be found at URL: http://hires.gsfc.nasa.gov/si/.

Paper Details

Date Published: 28 June 2006
PDF: 12 pages
Proc. SPIE 6268, Advances in Stellar Interferometry, 626821 (28 June 2006); doi: 10.1117/12.669713
Show Author Affiliations
Kenneth G. Carpenter, NASA Goddard Space Flight Ctr. (United States)
Carolus J. Schrijver, Lockheed Martin Advanced Technology Ctr. (United States)
Margarita Karovska, Smithsonian Astrophysical Observatory (United States)


Published in SPIE Proceedings Vol. 6268:
Advances in Stellar Interferometry
John D. Monnier; Markus Schöller; William C. Danchi, Editor(s)

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