Fin des années 1950, sous l'initiative de R.H. Dicke, la mesure télémétrique Terre-Lune fut initialement pensée pour tester la théorie de la Relativité Générale (RG) au travers de la variation de la constante gravitationnelle et du principe de Mach. Plus tard, K. Nordtvedt démontra qu'une telle expérience permettrait également de tester...
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July 2020 (v1)Journal articleUploaded on: December 4, 2022
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2019 (v1)Journal article
Lunar laser ranging (LLR) data and Apollo seismic data analyses, revealed independent evidence for the presence of a fluid lunar core. However, the size of the lunar fluid core remained uncertain by $\pm55$ km (encompassing two contrasting 2011 Apollo seismic data analyses). Here we show that a new description of the lunar interior's dynamical...
Uploaded on: December 3, 2022 -
2023 (v1)Journal article
Seismological models from Apollo missions provided the first records of the Moon inner structure with a decrease in seismic wave velocities at the core–mantle boundary1,2,3. The resolution of these records prevents a strict detection of a putative lunar solid inner core and the impact of the lunar mantle overturn in the lowest part of the Moon...
Uploaded on: May 11, 2023 -
April 23, 2023 (v1)Conference paper
The Moon is the most well-known extraterrestrial planetary body thanks to observations from ground-based, space-borne instruments and lunar surface missions. Data from Lunar Laser Ranging (LLR), magnetic, gravity, surface observations and seismic Apollo ground stations help us to quantify the deformation undergone by the Moon due to body tides....
Uploaded on: February 16, 2024 -
April 2023 (v1)Journal article
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Uploaded on: October 11, 2023 -
April 2023 (v1)Journal article
Abstract We investigate the impact of viscoelastic tidal deformation of the Moon on the motion of a polar orbiter. The dissipative effects in the Moon's interior, i.e., tidal phase lags, are modeled as Fourier series sampled at given frequencies associated with linear combinations of Delaunay arguments, the fundamental parameters describing the...
Uploaded on: October 11, 2023 -
October 12, 2018 (v1)Conference paper
Large (D>100km) asteroids are the most direct remnants of the building blocks of planets. (2) Pallas is the third largest asteroid and the parent body of a small collisional family. Its spectral properties indicate a B-type surface, meaning Pallas is most likely linked to carbonaceous chondrite meteorites. Disc-resolved images have revealed a...
Uploaded on: December 4, 2022