Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-30T23:44:32.570Z Has data issue: false hasContentIssue false
  • English
  • Français

Astrometry Using Interferometry at Optical Wavelengths

Published online by Cambridge University Press:  25 May 2016

K. J. Johnston ,
D. J. Hutter ,
J. A. Benson ,
N. M. Elias II ,
J. T. Armstrong ,
D. Mozurkewich ,
T. A. Pauls  and
C. A. Hummel
K. J. Johnston
Affiliation:
US Naval Observatory, USA
D. J. Hutter
Affiliation:
US Naval Observatory, USA
J. A. Benson
Affiliation:
US Naval Observatory, USA
N. M. Elias II
Affiliation:
US Naval Observatory, USA
J. T. Armstrong
Affiliation:
Naval Research Laboratory, USA
D. Mozurkewich
Affiliation:
Naval Research Laboratory, USA
T. A. Pauls
Affiliation:
Naval Research Laboratory, USA
C. A. Hummel
Affiliation:
Universities Space Research Association, USA

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.

Interferometry offers an improvement in the accuracy with which astrometric measurements can be made. Using this technique, radio astronomers together with geodeticists have established a global inertial reference frame that is accurate to 0.1 milliarcseconds. At optical wavelengths, interferometry was first developed by Michelson at the turn of the twentieth century, but due to the complexities of precise beam combination at high speeds, it has lagged in its development. Now, with the availability of lasers, detectors and computers that allow path length compensation on millisecond time scales and distance determination between light collectors with a precision of 0.01 μm, interferometry at optical wavelengths will achieve the results in astrometry comparable to those at radio wavelengths.

Type
Stellar Angular Diameters and Radii
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 39 - 44
Copyright
Copyright © Kluwer 1997 

References

Benson, J. A., Hutter, D. J., Elias, N. M. II, Bowers, P. F., Johnston, K. J., Hajian, A. R., Armstrong, J. T., Mozurkewich, D., Pauls, T. A., Rickard, L. J, Hummel, C. A., White, N. M., Black, D., & Denison, C. S. 1997, AJ, submitted Google Scholar
Brown, R. H., Davis, J., & Allen, R. L. 1974, MNRAS, 167, 121 Google Scholar
Colavita, M. M. 1994 A&A 283, 1027 Google Scholar
Hajian, A. R., et al. 1997, to be submitted to ApJ Google Scholar
Han, I. 1989, AJ, 97, 607 Google Scholar
Hummel, C. A., Armstrong, J. T., Buscher, D. F., Mozurkewich, D., Quirrenbach, A., & Vivekanand, M. 1995, AJ, 119, 376 CrossRefGoogle Scholar
Hummel, C. A., & Benson, J. A. 1997, this volume Google Scholar
Hummel, C. A., Mozurkewich, D., Elias, N. M. II, Quirrenbach, A., Buscher, D. F., Armstrong, J. T., Johnston, K. J., Simon, R. S. & Hutter, D. J. 1994, AJ, 108, 326 Google Scholar
Johnston, K. J., deVegt, C., Florkowski, D. M., & Wade, C. M. 1985, AJ, 90, 2390 Google Scholar
Johnston, K. J., Fey, A. L., Zacharias, N., Russell, J. L., Ma, C., deVegt, C., Reynolds, J. L., Jauncey, D. L., Archinal, B. A., Carter, M. S., Corbin, T. E., Eubanks, T. M., Florkowski, D. M., Hall, D. M., McCarthy, D. D., McCulloch, D. M., King, E. A., Nicholson, G., & Shaffer, D. B. 1995, AJ, 110, 880 Google Scholar
Lindegren, L. 1980, A&A, 89, 41 Google Scholar
Michelson, A. A. & Pease, F. G. 1921, ApJ, 53, 249 Google Scholar
Mozurkewich, D., Hutter, D. J., Johnston, K. J., Simon, R. S., Shao, M., Colavita, M. M., Staelin, D. H., Hines, B., Hershey, J. L., Hughes, J. A., & Kaplan, G. H. 1988, AJ, 95, 1296 CrossRefGoogle Scholar
Shao, M. & Staelin, D. H. 1980, J. Opt. Soc. Am., 19, 1519 Google Scholar
Shao, M., Colavita, M. M., Staelin, D. H., Johnston, K. J., Simon, R. S., Hughes, J. A. & Hershey, J. L. 1987, AJ, 93, 1280 Google Scholar
Thompson, A. R., Moran, J. M. & Swenson, G. W. 1986, Interferometry and Synthesis in Radio Astronomy (Wiley, New York)Google Scholar