An Introduction to the Space Interferometry Mission

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The Space Interferometry Mission will be the first spatial long-baseline optical interferometer in space. SIM is the first new mission in NASA's Origins program, following SIRTF. It is designed to perform wide-angle astrometry with 4 mu arcsec precision on objects as faint as V = 20, as well as synthesis imaging with 10 milliarcsec resolution, and interferometric nulling. As an example, this level of precision allows SIM to measure stellar parallax distances to 10%, and transverse velocities to 200 m/s, out to the far side of the Galaxy. This talk will explain the design and operation of this first-of-a kind mission. Precision astrometry is achieved by monitoring the fringe pattern on the detector, while a laser metrology system measures the delay difference between the light paths through the instrument. Imaging is done by rotational synthesis, analogous to the technique used by ground-based radio interferometer arrays. The basic architecture and observing techniques of SIM are scalable to much larger deployed structures in planned future missions.

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