SearcharxivSearch

arXiv subjects

Alex Guinard

Publications and source records attributed to Alex Guinard.

2 recordsLinked to original sources

NovaMoon: A Strategic Lunar Reference Station for Positioning, Timing, and Largely Enhanced Science in the Earth-Moon System

The renewed interest in lunar exploration and the development of future lunar communication and navigation services highlight the need for a precise, stable, and interoperable geodetic and timing infrastructure on the Moon. NovaMoon, proposed as a scientific and navigation payload for ESA's Argonaut lander, is designed as a lunar-based local differential, geodetic, and timing station supporting both operational needs in the Moon's south polar region and a broad range of scientific investigations. The payload integrates a lunar laser retroreflector, a Very Long Baseline Interferometry transmitter, a receiver for navigation signals compatible with LunaNet standards, high-stability atomic clocks, and direct-to-Earth radio links -- making it the first lunar station to co-locate multiple ranging, tracking, and timing techniques. NovaMoon will enable sub-metre to decimetre positioning, provide local differential corrections for lunar users, and ensure an accurate and stable realisation of position and time. Preliminary simulation studies show that this multi-technique dataset improves the lunar reference frame, orientation and ephemerides, and estimates of interior parameters like tidal response and core properties. NovaMoon will also provide the first long-duration physical realisation of a lunar time reference. Beyond its primary goals, it supports improved cartography, precise surface geolocation, and higher-resolution topography, contributing to safer landings and operations. It also enables new tests of fundamental physics, including constraints on relativity and possible deviations from classical gravity.

astro-ph.EP

Coupled geophysical and thermal constraints link between Mars basal molten layer and the planet viscosity profile

Computing the tidal deformations of Mars, we explored various Mars internal structures by examining profiles that include or exclude a basal molten layer within the mantle and a solid inner core. By assessing their compatibility with a diverse set of geophysical observations we show that despite the very short periods of excitation, tidal deformation is very efficient to constraint the Mars interior. We calculated densities and thicknesses for Martian lithosphere, mantle, {core-mantle boundary} layer and core and {found them} coherent with preexisting results from other methods. We also estimated new viscosities for these layers. We demonstrated that the geodetic record associated with thermal constraint is very sensitive to the {presence} of a basal molten layer in deep Martian mantle, and less sensitive to the solid core. Our results also indicate that the existence of the basal molten layer necessarily comes together with an inversion of viscosity between the lithosphere and the mantle. In this case, we could attribute this reverse viscosity contrast to the poor hydration state of Martian mantle and we underlined that this result prevents a strict Earth-like plate tectonics on Mars. The existence of the basal molten layer is also associated with a non-inversion of viscosity between the core-mantle boundary layer and the liquid core. Finally, in our results, a basal molten layer is incompatible with the existence of a solid inner core. Efforts to detect basal molten layer are then of prime importance to decipher the Martian interior. {Inversely, viscosity profiles appear to be very good tools for probing the existence of such molten layer at the base of the Mars mantle.

astro-ph.EP