Renard, Jean-Baptiste, Moussis, Olivier, Vaubaillon, Jérémie, Verdier, Nicolas, Berthet, Gwenaël, Levasseur-Regourd, Anny Chantal, Jorda, Laurent, Vernazza, Pierre, Zamkotsian, Frédéric, Geffrin, Jean-Michel, Eyraud, Christelle, Litman, Amelie, Tortel, Hervé, Rairoux, Patrick, Miffre, Alain, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), HIPE (HIPE), Institut FRESNEL (FRESNEL), Centre National de la Recherche Scientifique (CNRS)-École Centrale de Marseille (ECM)-Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS)-École Centrale de Marseille (ECM)-Aix Marseille Université (AMU), Institut Lumière Matière [Villeurbanne] (ILM), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-École Centrale de Marseille (ECM)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU)-École Centrale de Marseille (ECM)-Centre National de la Recherche Scientifique (CNRS), and Cardon, Catherine
International audience; The amount of interplanetary dust impacting the Earth’s atmosphere is still not well estimated, in terms oftotal mass, size distribution, and concentration of particles. We propose to apply the counting techniques usedin the Earth’s atmosphere for determining the concentration of liquid and solid aerosols, to the detection ofthese interplanetary particles. The main differences with the Earth’s atmosphere measurements are the very lowconcentrations, the high speed of the particles (at least several km/s) and the space conditions.We have developed recently an innovative design of aerosols counter, called LOAC, which provides the concen-trations for 19 size classes of particles in the 0.2-50 micrometer range, and also an estimate of their typology (ortheir light absorbing properties). The particles are injected through a laser beam via a pumping system, and twophotodiodes record the light scattered. This instrument combines the measurements at two different angles, thefirst at around 15° being insensitive to the refractive index and porosity of the particles, and the second one around60° being very sensitive to the nature of the particles. LOAC is used in routine since 5 years on the ground andfrom all kinds of balloons for the troposphere (mainly pollution) and stratosphere monitoring, and is also involvedin various international campaigns.An updated version of LOAC is in development for space applications, essentially for in situ measurementsplanetary atmospheres. LOAC can also be modified for the detection of high velocity particles, by using a lightsource of several cm long instead of a laser beam. No pump is needed, since the particles will cross an open celloriented at a constant angle from the motion of the instrument. This instrument could perform measurements inEarth orbit, onboard a micro-satellite or on the International Space Station.We will present this new concept of instrument, and how the measurements can be used to better constrain thenature and flux of the incoming interplanetary materia