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Interferometry Summer School

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Astrometric Interferometry in Space

Mike Shao (Jet Propulsion Laboratory)

Abstract:

This lecture will describe how space astrometry is conducted. Ground based interferometric astrometry is tied to the rotation of the Earth. In space, the platform (the spacecraft) is much less stable than the Earth, while at the same time, we want to achieve much higher accuracy. The lecture will describe how a space based astrometric interferometer would synthesize a microarcsec stable platform using "guide" stars and optical metrology. The 2nd major topic of the talk will be on systematic errors in space astrometric measurements. What types of instrumental errors are expected, how large instrumental biases can be corrected through calibration and "chopping".


Viewgraphs PDF 280k Bytes.
Viewgraphs PowerPoint 824k Bytes.
A note on the use of Summer School material.

Suggested Reading:

  • Long-Baseline Optical and Near-Infrared Interferometry
    M. Shao and M.M. Colavita,
    Ann. Rev. Astron. Astrophys. 30, 457-498 (1992).


2002 Home | Agenda | Participants | Reading | Software | Travel | Events | Local Guide

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Course Notes from the 2002 Michelson Interferometry Summer School
Smithsonian Astrophysical Observatory, Cambridge Massachusetts, June 24-28, 2002

Edited by P.R. Lawson (JPL), MS 301-451 Jet Propulsion Laboratory
Pasadena, California, 91109
Last Updated 9 February 2004

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