The effect of UV reflected back from the lunar surface on the detection of dust particles by the LDEX (Lunar Dust EXperiment) instrument

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[6250] Planetary Sciences: Solar System Objects / Moon

Scientific paper

The Lunar Dust EXperiment (LDEX) instrument is under development for the Lunar Atmosphere and Dust Environment Explorer (LADEE) to be launched in 2012. The LDEX instrument is designed to map the properties and temporal and spatial variations of the dust population in the vicinity of the Moon. The operation of the instrument is based on the impact ionization process, where free electrons and ions are generated upon the hypervelocity impact of the dust on a hemispherical target surface. The electrons and ions are separated by electric field and measured on the target and a microchannel plate (MCP) detector, respectively. The total charge is a measure of the dust mass and impact velocity. LADEE will orbit the Moon with small inclination (<20 degree) in the retrograde direction and LDEX will be pointed in the ram direction to sample the dust. The UV radiation from the Sun or reflected from the lunar surface can enter the LDEX instrument and will generate noise and thus limit the lower detection threshold of dust particles. In this paper we present the modeling of UV radiation reaching the MCP detector on different parts of the orbit. The modeling is performed by using the Zemax ray-tracing software. The preliminary results indicate that the detection limit will be > 0.25 micron radius dust for single impact detection. The results are also used to define the required optical properties of surfaces used in the LDEX instrument.

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