Thanks to NARVAL, the Bernard Lyot Telescope is now the leading observatory in the world dedicated to this type of study. And, since the Sun sets in Hawaii when it is rising in the Pyrenees, when NARVAL and ESPaDOnS work together they do not miss a single iota of the secrets of the magnetic life of the stars!

"Magnetic fields are essential ingredients in the life of stars. They are not only tracers of their history but also play a key role in their evolution" explains Pascal Petit, astronomer at the Laboratoire d'Astrophysique de Toulouse-Tarbes (LATT, Astrophysics Laboratory of Toulouse-Tarbes: CNRS, UPS (Paul Sabatier University), OMP (Pic du Midi Observatory)) and Scientific Director of NARVAL. "It is thought, for example, that the Sun's magnetic field could be at the origin of the Little Ice Age, the period of intense cold that gripped Europe during the reign of Louis XIV (1643-1715). Even more spectacular: magnetic fields are capable of upsetting the birth of stars by modifying the quantity of material from which they form. However, at the moment, relatively little is known of these magnetic fields -- even the Sun's magnetic field remains a mystery to us!" And, according to Michel Aurière of the LATT, NARVAL project leader "Thanks to NARVAL, we now have a telescope equipped with an instrument dedicated to the study of the magnetic fields of stars. Until now, ESPaDOnS was only available for a small proportion of the time, sharing nights at the Canada-France-Hawaii Telescope with other much sought after instruments. The arrival of NARVAL, a twin copy of ESPaDOnS, will allow French and international astronomers to redouble their efforts and to conduct much more ambitious projects than ever before." David Mouillet, Director of the Bernard Lyot Telescope (TBL) until the end of 2006, adds "Scientists from several countries have not been mistaken in taking the telescope by storm as soon as it was made available to the scientific community!"

To demonstrate the power of NARVAL and the important contribution it can make, SU Aurigae, an infant star located 450 light years from the Sun, was continuously scanned both by NARVAL and by ESPaDOnS within the scope of an international collaboration involving the LATT, the Laboratoire d'Astrophysique de Grenoble (LAOG, Astrophysics Laboratory of the Observatory of Grenoble, (CNRS/UJF (Joseph Fourier University)) and several British laboratories. "Only several million years old, SU Aurigae is around 1000 times younger than the Sun" explains Jean-François Donati, CNRS Research Director and the designer of ESPaDOnS and NARVAL. "At that age, a star is not yet fully formed and it continues to attract the material that surrounds it. Once captured in the magnetic ‘web', the material is then drained towards the star along the field lines, like pearls on a necklace. These observations suggest that SU Aurigae's magnetic ‘web' is a lot more complex than was initially predicted by stellar formation models."

The NARVAL project is being led by the technical team of the TBL and the LATT. It has benefited from the scientific and technical expertise, unique in the world, which the Toulouse-based research team has built up in the field of astronomic spectropolarimetry over the last decade. Costing a total of around 1 M €, NARVAL was funded by the Région Midi-Pyrénées (Midi-Pyrénées Region) and the Ministère de la Recherche (French Ministry of Research) (within the scope of a CPER (French State Region Planning Contract)), the Conseil Général des Hautes Pyrénées (Hautes-Pyrénées General Council), the European Union (FEDER funds) and CNRS' Institut National des Sciences de l'Univers (INSU, French National Institute for Sciences of the Universe).

The complex network of magnetic field lines emanating from the surface of the infant star SU Aurigae as observed by NARVAL.

Source: CNRS