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A Planet in a Circular Orbit with a 6 Year Period*

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Published 2003 July 16 © 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Brad D. Carter et al 2003 ApJ 593 L43 DOI 10.1086/378185

1538-4357/593/1/L43

Abstract

Precision Doppler velocity measurements from the 3.9 m Anglo-Australian Telescope reveal a planet with a 6 yr period orbiting the G5 dwarf HD 70642. The a = 3.3 AU orbit has a low eccentricity (e = 0.1), and the minimum (M sin i) mass of the planet is 2.0MJUP. The host star is metal-rich relative to the Sun, similar to most stars with known planets. The distant and approximately circular orbit of this planet makes it a member of the rarest group to emerge from precision Doppler surveys.

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Footnotes

  • Based on observations obtained at the Anglo-Australian Telescope, Siding Spring, Australia.

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10.1086/378185