Breakthrough capability for UVOIR space astronomy: reaching the darkest sky

We describe how availability of new solar electric propulsion (SEP) technology can substantially increase the science capability of space astronomy missions working within the near-UV to far-infrared (UVOIR) spectrum by making dark sky orbits accessible for the first time. We present two case studies in which SEP is used to enable a 700 kg Explorer-class and 7000 kg flagship-class observatory payload to reach an orbit beyond where the zodiacal dust limits observatory sensitivity. The resulting scientific performance advantage relative to a Sun-Earth L2 point (SEL2) orbit is presented and discussed. We find that making SEP available to astrophysics Explorers can enable this small payload program to rival the science performance of much larger long development-time systems. Similarly, we find that astrophysics utilization of high power SEP being developed for the Asteroid Redirect Robotics Mission (ARRM) can have a substantial impact on the sensitivity performance of heavier flagship-class astrophysics payloads such as the UVOIR successor to the James Webb Space Telescope.

[1]  Dale J. Fixsen,et al.  The Zodiacal Emission Spectrum as Determined by COBE and Its Implications , 2002 .

[2]  Robert D. Falck,et al.  Extra-Zodiacal-Cloud Astronomy via Solar Electric Propulsion , 2011 .

[3]  D. J. Fixsen,et al.  Breakthrough capability for the NASA astrophysics explorer program: reaching the darkest sky , 2012, Other Conferences.

[4]  Mark Clampin,et al.  Individual photon counting using e2v L3 CCDs for low background astronomical spectroscopy , 2006, SPIE Astronomical Telescopes + Instrumentation.

[5]  Angioletta Coradini,et al.  Exploring the asteroid belt with ion propulsion: Dawn mission history, status and plans , 2007 .

[6]  Chuck Lillie,et al.  A mission architecture for future space observatories optimized for SAFIR , 2005, SPIE Optics + Photonics.

[7]  E. L. Wright,et al.  The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. II. Model of the Interplanetary Dust Cloud , 1997, astro-ph/9806250.

[8]  B. Bumble,et al.  ARCONS: A 2024 Pixel Optical through Near-IR Cryogenic Imaging Spectrophotometer , 2013, 1306.4674.

[9]  Wesley A. Traub,et al.  Advanced Technology Large-Aperture Space Telescope: science drivers and technology developments , 2012 .

[10]  E. Figueroa-Feliciano,et al.  First astronomical application of a cryogenic transition edge sensor spectrophotometer , 1999 .

[11]  David Schiminovich,et al.  Delta-doped electron-multiplied CCD with absolute quantum efficiency over 50% in the near to far ultraviolet range for single photon counting applications. , 2012, Applied optics.