The catalogue of extrasolar planets is growing continuously, containing today more than 200 objects, and the detection of these exoplanets has almost become a routine. But what are the characteristics of the stellar hosts, how can we explain the formation of these planetary systems, or why are some of these giant exoplanets, which are called 'hot jupiters', migrating down to very close-in orbits? Astrophysicists suspect the magnetic field to play a crucial role in some of these questions. However, although indirect effects of magnetic fields have already been detected on stars hosting giant extrasolar planets, no direct measurement had ever been done until now.
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Artist
view of the giant exoplanet orbitng tau Bootis, through the star's
magnetic archs (credit David Aguilar, CfA)
This first measurement of a magnetic field in a planet-hosting star has been obtained by an international team of astronomers with the ESPaDOnS spectropolarimeter located on the Canada-France-Hawaii telescope. They detected the magnetic field of tau Bootis, a one billion year old star, having a mass of one and a half solar masses and located at nearly 50 light years from the Earth. This cool and weakly active star, orbited by a giant planet with 4.4 Jupiter masses on a very close-in orbit at 0.049 AU (i.e. 5% of the Sun-Earth distance), possesses a magnetic field of a few gauss, just a little more than the Sun's, but showing a more complex structure.
Moreover, astronomers have also measured the level of differential rotation of the star, a crucial parameter in the generation of magnetic fields. In the present case, the matter located at the equator rotates 18% faster than that located at the poles, leading by one full turn in approximately 15 days. By comparing the differential rotation of the star with the revolution of the giant extrasolar planet, astronomers have noticed that the planet is synchronized with stellar material located at about 45 degrees. This observation suggests very complex interactions between the magnetosphere of the star and its companion, perhaps similar to the interaction of the magnetosphere of Jupiter with its satellite Io, giving rise to the so-called "Io torus".
The data collected for this study are not sufficient to describe precisely these interactions, but this first measurement is opening new prospects for detailed studies of star-planet systems.
Press release written by Cyrille Baudouin, with the support of SF2A (Société
Française d'Astronomie et d'Astrophysique)
Notes:
(1) ESPaDOnS is a collaborative project funded by France (CNRS/INSU,
Ministère de la Recherche, LATT - Observatoire Midi
Pyrénées,
Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique -
Observatoire de Paris), Canada ((NSERC), CFHT and ESA (ESTEC/RSSD).
(2) CFHT is operated by the National Research Council of Canada, the
Institut National des Sciences de l’Univers of the Centre National de
la Recherche Scientifique of France, and the University of Hawaii.
Reference:
The magnetic field of the planet-hosting star tau Bootis
C. Catala, J-F. Donati, E. Shkolnik, D. Bohlender, E. Alecian
2006, MNRAS, in
press
Contact
Claude
Catala (Observatoire de Paris, LESIA et CNRS)
Jean-Francois Donati, (LATT) - jean-francois.donati @ ast.obs-mip.fr
Evelyne
Alecian (Observatoire de Paris, LESIA et CNRS)
For more information on ESPaDOnS at CFHT
Nadine Manset, CFHT - manset @ cfht.hawaii.edu - 808 885 7944
Christian Veillet, CFHT - veillet @ cfht.hawaii.edu - 808 938 3905