The 2:1 Resonant Exoplanetary System Orbiting HD 73526*

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© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation C. G. Tinney et al 2006 ApJ 647 594 DOI 10.1086/503706

0004-637X/647/1/594

Abstract

We report the detection of a second exoplanet orbiting the G6 V dwarf HD 73526. This second planet has an orbital period of 377 days, putting it in a 2 : 1 resonance with the previously known exoplanet, the orbital period for which is updated to 188 days. Dynamical modeling of the combined system allows solution for a self-consistent set of orbital elements for both components. HD 73526 is the fourth exoplanetary system (of a total of 18 systems with two or more components currently known) to have components detected in 2 : 1 resonance. Finding such a large fraction of multiple planets (more than 20%) in 2 : 1 resonance strongly suggests that orbital migration, halted by stabilization in a trapping resonance, plays an important role in the evolution of exoplanets in multiple planet systems.

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Footnotes

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

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10.1086/503706