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direct imaging of stellar surfaces: results from the stellar imager (si) vision mission studyThe Stellar Imager (SI) is a UV-Optical, Space-Based Interferometer designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and stellar interiors (via asteroseismology) and of the Universe in general. 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). The ultra-sharp images of the Stellar Imager will revolutionize our view of many dynamic astrophysical processes: The 0.1 mas resolution of this deep-space telescope 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 in support of the Living With a Star program in the Exploration Era. 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. In this paper we will discuss the results of the SI Vision Mission Study, elaborating on the science goals of the SI Mission and a mission architecture that could meet those goals.
Document ID
Document Type
Conference Paper
Carpenter, Kenneth
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Schrijver, Carolus
(Lockheed Martin Advanced Technology Center United States)
Karovska, Margarita
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2006
Subject Category
Meeting Information
Cool Stars Workshop (poster presentation)(Pasadena, CA)
Distribution Limits
Work of the US Gov. Public Use Permitted.