Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-17T18:18:42.174Z Has data issue: false hasContentIssue false

Astrometry with SIM PlanetQuest

Published online by Cambridge University Press:  01 October 2007

M. Shao*
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91007, USA email: Michael.Shao@jpl.nasa.gov
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

SIM PlanetQuest is a very high accuracy space astrometric instrument based on a long baseline stellar interferometer. For global astrometry SIM was designed to be accurate to ≈ 4μas (microarcsec) after a 5 year mission. For narrow angle astrometry (≈ 1000 s integration over a 1° radius field) SIM is designed for 1μas precision. The technology program was completed in 2005 and based on laboratory results, the current best estimate of SIM's performance would be 0.6 μas for narrow angle precision and 2.4 μas for global accuracy. This paper describes a variety of science programs that the SIM science team have proposed to conduct from a search for one Earth mass planets in the habitable zone of (≈130) nearby stars to the study of dark matter in the galactic disk, the galactic halo and the local group.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Beichman, C. 2008, Proceedings of IAU Symposium 248, in this volume p.238Google Scholar
Chaboyer, B. 2008, Proceedings of IAU Symposium 248, in this volume p.440Google Scholar
Hines, B., et al. 2003, SPIE, vol. 4852, p45Google Scholar
Majewski, S. 2008, Proceedings of IAU Symposium 248, in this volume p.450Google Scholar
Unwin, S. 2008, Proceedings of IAU Symposium 248, in this volume p.288CrossRefGoogle Scholar
Unwin, S. et al. 2007, PASP, acceptedGoogle Scholar