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The HARPS search for southern extra-solar planets - XVIII. An Earth-mass planet in the GJ 581 planetary system
Michel Mayor, X. Bonfils, T. Forveille, X. Delfosse, Stephane Udry, Jean-Loup Bertaux, H. Beust, François Bouchy, C. Lovis, Francesco Pepe, C. Perrier, Didier Queloz, N.C. Santos

The HARPS search for southern extra-solar planets - XVIII. An Earth-mass planet in the GJ 581 planetary system

Science & Mathematics Published 2009 Verification Pending

Overview & Synopsis

The GJ 581 planetary system is already known to harbour three planets, including two super-Earth planets that straddle its habitable zone. We report the detection of an additional planet - GJ 581e - with a minimum mass of 1.9 $M_\oplus$. With a period of 3.15 days, it is the innermost planet of the system and has a ~5% transit probability. We also correct our previous confusion about the orbital period of GJ 581d (the outermost planet) with a one-year alias, benefitting from an extended time span and many more measurements. The revised period is 66.8 days, and positions the semi-major axis inside the habitable zone of the low mass star. The dynamical stability of the 4-planet system imposes an upper bound on the orbital plane inclination. The planets cannot be more massive than approximately 1.6 times their minimum mass.

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Document Information

Document Title The HARPS search for southern extra-solar planets - XVIII. An Earth-mass planet in the GJ 581 planetary system
Author / Organization Michel Mayor, X. Bonfils, T. Forveille, X. Delfosse, Stephane Udry, Jean-Loup Bertaux, H. Beust, François Bouchy, C. Lovis, Francesco Pepe, C. Perrier, Didier Queloz, N.C. Santos
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2009
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-241253
Original Source Link Visit Source Page on hal.science »