activity
20112022
most citedScientific rationale for Uranus and Neptune in situ explorations

100 citations · 618 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2022★ 5 cited

Detection and characterization of wind-blown charged sand grains on Titan with the DraGMet/EFIELD experiment on Dragonfly

Audrey Chatain, Alice Le Gall, Jean-Jacques Berthelier +5

The EFIELD instrument is part of the geophysics and meteorology sensor package DraGMet on the Dragonfly mission, which will explore the surface of Titan in the mid-2030s. EFIELD co…

astro-ph.EP2022

Moonraker -- Enceladus Multiple Flyby Mission

O. Mousis, A. Bouquet, Y. Langevin +50

Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could b…

astro-ph.EP2021★ 1 cited

Science goals and new mission concepts for future exploration of Titan's atmosphere geology and habitability: Titan POlar Scout/orbitEr and In situ lake lander and DrONe explorer (POSEIDON)

Sébastien Rodriguez, Sandrine Vinatier, Daniel Cordier +61

In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest m…

astro-ph.EP2017★ 100 cited

Scientific rationale for Uranus and Neptune in situ explorations

O. Mousis, D. H. Atkinson, T. Cavalié +53

The ice giants Uranus and Neptune are the least understood class of planets in our solar system but the most frequently observed type of exoplanets. Presumed to have a small rocky…

physics.space-ph2017★ 21 cited

Cold and warm electrons at comet 67P

A. I. Eriksson, I. A. D. Engelhardt, M. Andre +20

Strong electron cooling on the neutral gas in cometary comae has been predicted for a long time, but actual measurements of low electron temperature are scarce. We present in situ…

physics.space-ph2016★ 88 cited

Spatial distribution of low-energy plasma around comet 67P/CG from Rosetta measurements

N. J. T. Edberg, A. I. Eriksson, E. Odelstad +22

We use measurements from the Rosetta plasma consortium (RPC) Langmuir probe (LAP) and mutual impedance probe (MIP) to study the spatial distribution of low-energy plasma in the nea…

physics.space-ph2015★ 72 cited

Observation of a New Type of Low Frequency Waves at Comet 67P/Churyumov-Gerasimenko

I. Richter, C. Koenders, H. -U. Auster +23

We report on magnetic field measurements made in the innermost coma of 67P/Churyumov-Gerasimenko in its low activity state. Quasi-coherent, large-amplitude (), compres…

astro-ph.EP2014★ 64 cited

Scientific rationale of Saturn's in situ exploration

O. Mousis, L. N. Fletcher, J. -P. Lebreton +47

Remote sensing observations meet some limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. A remarkable example of the superior…

astro-ph.IM2013★ 20 cited

Fast E-sail Uranus entry probe mission

Pekka Janhunen, Jean-Pierre Lebreton, Sini Merikallio +3

The electric solar wind sail is a novel propellantless space propulsion concept. According to numerical estimates, the electric solar wind sail can produce a large total impulse pe…

astro-ph.SR2013★ 67 cited

Modeling the HD32297 Debris Disk with Far-IR Herschel Data

J. K. Donaldson, J. Lebreton, A. Roberge +2

HD32297 is a young A-star (~30 Myr) 112 pc away with a bright edge-on debris disk that has been resolved in scattered light. We observed the HD32297 debris disk in the far-infrared…

astro-ph.IM2013★ 57 cited

Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy

O. Mousis, R. Hueso, J. -P. Beaulieu +57

Amateur contributions to professional publications have increased exponentially over the last decades in the field of Planetary Astronomy. Here we review the different domains of t…

astro-ph.SR2012★ 36 cited

Hot circumstellar material resolved around beta Pic with VLTI/PIONIER

D. Defrère, J. Lebreton, J. -B. Le Bouquin +11

We aim at resolving the circumstellar environment around beta Pic in the near-infrared in order to study the inner planetary system (< 200 mas, i.e., ~4 AU). Precise interferometri…

astro-ph.EP2011★ 87 cited

Hot exozodiacal dust resolved around Vega with IOTA/IONIC

D. Defrère, O. Absil, J. -C. Augereau +10

Although debris discs have been detected around a significant number of main-sequence stars, only a few of them are known to harbour hot dust in their inner part where terrestrial…