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Anisotropy in the aberration constant due to galactic rotation

  • Fundamental Aspects of Metrology
  • Published:
Measurement Techniques Aims and scope

Abstract

It is shown that in the near future it will be possible to detect the dependence of the aberration constant on the direction to a star caused by our secular rotation. The corresponding corrections to the visible stellar positions will increase the accuracy in determining the Earth's rotation parameters by astro-optical means.

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Authors
  1. A. A. Grishaev
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Additional information

Traslated from Izmeritel'naya Tekhnika, No. 3 pp. 12–13, March, 1994.

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Grishaev, A.A. Anisotropy in the aberration constant due to galactic rotation. Meas Tech 37, 253–255 (1994). https://doi.org/10.1007/BF02614260

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  • DOI: https://doi.org/10.1007/BF02614260

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