The dwarf that carries a world

November 30, 2005

A team of French and Swiss astronomers [1] have discovered one of the lightest exoplanets ever found using the HARPS instrument [2] on ESO's 3.6-m telescope at La Silla (Chile). The new planet orbits a star belonging to the class of red dwarfs. As these stars are very common, this discovery proves crucial in the census of other planetary systems.

"Our finding possibly means that planets are rather frequent around the smallest stars," says Xavier Delfosse, from the Laboratoire d'Astrophysique de Grenoble (France) and co-author of the paper relating the work. "It certainly tells us that red dwarfs are ideal targets for the search for exoplanets."

The host star, Gl 581 [3], is located 20.5 light-years away in the Libra constellation (The Scales), and has a mass of only one third the mass of the Sun. Such red dwarfs are at least 50 times fainter than the Sun and are the most common stars in our Galaxy: among the 100 closest stars to the Sun, 80 belong to this class.

Being so numerous in our vicinity, it is thus fundamental to know if such stars also harbour planets. Previous surveys were rather unsuccessful: observations of about 200 red dwarfs revealed only 2 with planets.

"But previous surveys may have missed many planets due to their insufficient precision," says Stéphane Udry, from the Geneva Observatory and co-author of the work. "This is why we decided to make use of the ultra-precise, second generation, HARPS spectrograph. Our new result indicates this was the right strategy."

The newly found planet is about 17 times the Earth's mass, or about the mass of Neptune. It is therefore one of the smallest ever found [4]. It is rather close to its host star and completes a full circle in only 5.4 days: the mean distance is about 6 million kilometres. By comparison, Mercury, the closest planet to the Sun, is at a distance of 58 million kilometres and completes an orbit in 88 days. Being so close, this alien world must be very hot, about 150 degrees.

The planet was revealed by the wobble it induces on the host star. With the HARPS very precise measurements, the astronomers found the star to move back and forth with a maximum velocity of 13 metres/second, or a little bit less than 50 km/h.
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The astronomers have published their results in a Letter to the Editor of Astronomy and Astrophysics ("The HARPS search for southern extra-solar planets. VI. A Neptune-mass planet around the nearby M dwarf Gl 518", by X. Bonfils et al., A&A 443, L15, 2005).

Notes
[1]: The team is composed of Xavier Bonfils (Laboratoire d'Astrophysique de Grenoble (LAOG), France, and Geneva Observatory, Switzerland), Thierry Forveille (CFHT Corporation, Hawaii, USA and LAOG), Xavier Delfosse and Christian Perrier (LAOG), Stéphane Udry, Michel Mayor, Francesco Pepe, and Didier Queloz (Geneva Observatory), François Bouchy (Laboratoire d'Astrophysique de Marseille, France), and Jean-Louis Bertaux (Service d'Aéronomie du CNRS, France).

[2]: HARPS (High Accuracy Radial Velocity for Planetary Searches) is the most precise spectrograph to date, measuring radial velocities with a precision better than 1 m/s, or 3.6 km/h.

[3]: Gl 581, or Gliese 581, is the 581th entry in the Gliese Catalogue, which lists all known stars within 25 parsecs (81.5 light years) of the Sun. It was originally compiled by Gliese and published in 1969, and later updated by Gliese and Jahreiss in 1991.

[4]: Of the 170 exoplanets known today, 5 are possibly less massive than the one orbiting Gl 581: Gliese 876d (7.3 Earth's masses, or 7.3 ME), HD 160691 d (14 ME), 55 Cnc e (14.4 ME), HD 212301 b (14.4 ME) and HD 4308 b (15 ME). The masses indicated are in fact minimum masses, as the inclination of the system is unknown. One Jupiter mass is 18.6 Neptune masses or 319 Earth masses.

Additional Contacts
Xavier Delfosse
LAOG, France
Phone: 33-47-663-5510
Email: Xavier.Delfosse@obs-ujf-grenoble.fr

Stephane Udry
Geneva Observatory, Switzerland
Phone: 41-22-755-2611
Email: Stephane.Udry@obs.unige.ch

ESO

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