Interplanetary dust and debris, as observed from the Moon

Astronomy and Astrophysics – Astronomy

Scientific paper

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Interplanetary Dust, Lunar Bases, Space Debris, Zodiacal Light, Astronomical Polarimetry, Radiation Sources, Satellite Observation, Moon, Space, Utilization, Astronomy, Science Aspects, Zodiacal Light, Interplanetary Dust, Idps, Photopolarimetry, Satellite Observations, Moon-Based Observations, Thermal Emissions, Grains, Particles, Flux, Impact Effects, Micrometeorites, Size Distribution, Emissions, Atmosphere, Wavelength, Near Infrared, Visible Light

Scientific paper

The visible trace of the interplanetary dust cloud, so-called the zodiacal light, has already been photographed from the Moon, more than twenty years ago (part 1). The interplanetary dust grains do not only scatter solar light; they produce a thermal emission in the near infrared domain; also they may impact the Earth and Moon system as they spiral towards the Sun (part 2). The main problems which can be anticipated for Moon based observations of faint astronomical sources are likely to be due to zodiacal light and zodiacal emission; the induced contamination would however be reduced by appropriate choices in the periods of observation (part 3).

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