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The HARPS survey for southern extra-solar planets

Title
The HARPS survey for southern extra-solar planets
Type
Article in International Scientific Journal
Year
2004
Authors
N.C. Santos
(Author)
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Bouchy, F
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Mayor, M
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Pepe, F
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Queloz, D
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Udry, S
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Lovis, C
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Bazot, M
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Benz, W
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Bertaux, J
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Lo Curto, G
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Delfosse, X
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Mordasini, C
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Naef, D
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Sivan, J
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Vauclair, S
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Journal
Vol. 426
Pages: L19-L23
ISSN: 0004-6361
Publisher: EDP Sciences
Other information
Authenticus ID: P-00H-KQM
Abstract (EN): In this letter we present the discovery of a very light planetary companion to the star mu Ara (HD160691). The planet orbits its host once every 9.5 days, and induces a sinusoidal radial velocity signal with a semi-amplitude of 4.1 m s(-1), the smallest Doppler amplitude detected so far. These values imply a mass of m(2) sin i = 14 M-circle times (Earth-masses). This detection represents the discovery of a planet with a mass slightly smaller than that of Uranus, the smallest "ice giant" in our Solar System. Whether this planet can be considered an ice giant or a super-earth planet is discussed in the context of the core-accretion and migration models.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 5
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