In 1972, astronauts on board Apollo 17 saw a lunar sunrise while they were in orbit around the Moon. They made drawings of the distribution of light above the lunar horizon, which has been called "the lunar sunrise sketches". The sunrise sketches by the Apollo 17 crew have been interpreted to contain light scattered by interplanetary dust as well as light scattered by dust in the close vicinity of Moon. In this thesis the light scattering by interplanetary dust and by a micrometeoroid impact-generated lunar ejecta cloud at the time of Apollo 17 sunrise sketches is modeled and an image is reconstructed for the same observation geometry that can be compared to the sunrise sketches. To determine the contribution of light scattered by different...
Photometric and meteor observations, scattering properties, particle collection and impact, solar wi...
We have developed a scattering model allowing to study interaction of light with particles populatin...
For certain combinations of lighting and viewing conditions, the lunar landing site will be void of ...
The lunar horizon glow observed by Apollo astronauts and recorded during the Surveyor missions is be...
Planetary bodies throughout the solar system are continually bombarded by dust particles, largely or...
Space dust consists of particles typically 0.1 mm in diameter or less. They overlap with the sizes o...
Estimating the sky background is critical for ground-based astronomical research. In the optical, sc...
International audienceThis chapter reviews how the polarization of light scattered by interplanetary...
The largest natural source of light at night is the Moon, and it is the major contributor to the ast...
International audienceThe zodiacal light is a night-glow mostly visible along the plane of the eclip...
The largest natural source of light at night is the Moon, and it is the major contributor ...
Humanity is on course to return to the surface of the Moon within the next decade, with plans and as...
International audienceStudying intensity and linear polarization of the solar light scattered by int...
Photometric and meteor observations, scattering properties, particle collection and impact, solar wi...
We have developed a scattering model allowing to study interaction of light with particles populatin...
For certain combinations of lighting and viewing conditions, the lunar landing site will be void of ...
The lunar horizon glow observed by Apollo astronauts and recorded during the Surveyor missions is be...
Planetary bodies throughout the solar system are continually bombarded by dust particles, largely or...
Space dust consists of particles typically 0.1 mm in diameter or less. They overlap with the sizes o...
Estimating the sky background is critical for ground-based astronomical research. In the optical, sc...
International audienceThis chapter reviews how the polarization of light scattered by interplanetary...
The largest natural source of light at night is the Moon, and it is the major contributor to the ast...
International audienceThe zodiacal light is a night-glow mostly visible along the plane of the eclip...
The largest natural source of light at night is the Moon, and it is the major contributor ...
Humanity is on course to return to the surface of the Moon within the next decade, with plans and as...
International audienceStudying intensity and linear polarization of the solar light scattered by int...
Photometric and meteor observations, scattering properties, particle collection and impact, solar wi...
We have developed a scattering model allowing to study interaction of light with particles populatin...
For certain combinations of lighting and viewing conditions, the lunar landing site will be void of ...