The emission of dust particles in the interstellar medium of our galaxy and nearby galaxies is slightly polarized, as the particles are elongated and aligned with the magnetic field that prevails in the interstellar medium. The measurements obtained by Pilot will help scientists understand the nature of dust particles and why they are aligned in this way. The measurements will also be used to map the geometry of the magnetic field, which plays an important part in contracting the gas in the interstellar medium, a phenomenon that leads to the formation of new stars.
This emission is also an obstacle for experiments that seek to accurately measure the polarization of the cosmic microwave background, and Pilot's measurements will shed more light on it, and thus improve the interpretation of the results obtained with this type of experiment.
The Pilot experiment will observe this emission in the far infrared region. It is equipped with 2,048 individual detectors, cooled to a temperature of 300 millikelvin, i.e. close to absolute zero. Polarization is measured using a rotating blade and a polarizer that separates two orthogonal polarizations on the two focal planes of the experiment. Apart from the primary mirror of the telescope, all the optics is maintained at a cryogenic temperature (2 kelvins or -271°C) inside a cryostat, cooled with liquid helium, to limit the instrument's own emission.
The experiment was conceived and built by CNRS scientists and engineers at the Research Institute in Astrophysics and Planetology (CNRS/CNES/Paul Sabatier University) and IAS (CNRS/Paris-Sud University), with major contributions from the CNES Balloon Division in Toulouse, the ESA, the CEA (Saclay), which developed the focal plane and its electronics, La Sapienza University in Rome (Italy), and Cardiff University (United Kingdom). The whole project is backed by CNRS laboratories and CNES funding.
In a few days, Pilot will be launched by CNES as part of a campaign comprising three flights with different gondolas from Alice Springs, in central Australia. Pilot weighs nearly one metric ton and will have to climb to an altitude of nearly 40 km. It therefore requires the use of an open stratospheric balloon, approximately 100 m in diameter (the largest open balloon ever launched by CNES), and a payload chain as tall as the Eiffel Tower.
The flight will take place during one of the two annual reversals of stratospheric winds, which is a prerequisite for any hope of performing observations for more than 30 hours at the ceiling altitude. Although Pilot has already been launched in the past - its first flight was from Canada in September 2015 - this new flight will be in the southern hemisphere, thus providing an opportunity to observe outstanding astrophysical sources, such as the Magellanic Clouds, satellite galaxies of our own galaxy, or inner regions of the Milky Way, that cannot be observed from the northern hemisphere.
The PILOT scientific instrument after integration in the NASA building in Alice Springs (Australia).
The front baffle is designed to attenuate stray light due to the thermal emission of the Earth and the envelope
of the stratospheric balloon.
© Sébastien Chastanet - OMP / IRAP / UT3 / CNES / CNRS
The PILOT experiment beneath the Australian sky during night-time tests on the Estadius stellar sensor. The PILOT instrument
will observe some of the regions of the Milky Way that can be seen in this photo.
© Sébastien Chastanet - OMP / IRAP / UT3 / CNES / CNRS