The 2:1 resonant exoplanetary system orbiting HD 73526

Tinney, C. G. and Butler, R. Paul and Marcy, Geoffrey W. and Jones, Hugh R. A. and Laughlin, Gregory and Carter, Brad D. and Bailey, Jeremy and O'Toole, Simon J. (2006) The 2:1 resonant exoplanetary system orbiting HD 73526. The Astrophysical Journal, 647 (1). pp. 594-599. ISSN 0004-637X

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Official URL: http://www.journals.uchicago.edu/doi/pdf/10.1086/503706

Abstract

[Abstract]: We report the detection of a second exoplanet orbiting the G6V dwarf HD73526. This second planet has an orbital period of 377 d, putting it in a 2:1 resonance with the previously known exoplanet, the orbital period for which is updated to 188 d. Dynamical modeling of the combined system allows solution for a self-consistent set of orbital elements for both components. HD73526 is the fourth exoplanetary system (of a total of 18 systems with 2 or more components currently known) to have components detected in 2:1 resonance. Finding such a large fraction of multiple planets (more than 20 per cent) in 2:1 resonance strongly suggests that orbital migration, halted by stabilisation in a trapping resonance, plays an important role in the evolution of exoplanets in multiple planet systems.

Item Type:Article (DEST Category C)
Additional Information:Published version deposited in accordance with the copyright policy of the publisher.
Uncontrolled Keywords:planetary systems, stars, HD73526
Fields of Research (FOR2008):UNSPECIFIED
Subjects:240000 Physical Sciences > 240100 Astronomical Sciences
Socio-Economic Objective (SEO2008):UNSPECIFIED
ID Code:2052
Deposited By:epEditor USQ
Deposited On:11 Oct 2007 10:56
Last Modified:28 May 2009 10:14

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