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Astrometry is the oldest search method for extrasolar planets and originally popular because of its success in characterizingastrometricbinarystar systems.
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This star is a suspectedastrometricbinary, although nothing is known about the companion.
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This is anastrometricbinarysystem with a period of 6.5 years (2,374 days) and an orbital eccentricity of 0.10.
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This is anastrometricbinarysystem.
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Combining this with other proper motion data spanning approximately half a century indicated a periodic variation of 26.5 2 years, confirming that the star is anastrometricbinary.
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