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PUBLICATIONS

Saturn's formation and early evolution at the origin of Jupiter's massive moons

Here we have investigated the origin and delivery of the building blocks of the Galilean satellites, the four most massive jovian moons.

T. Ronnet, O. Mousis, P. Vernazza, J. I. Lunine, A. Crida 2018, AJ.

Pebble accretion at the origin of Europa's water

T. Ronnet, O. Mousis & P. Vernazza 2017, ApJ.

Europa is one of the four massive Galilean satellites orbiting around Jupiter. A water ocean lies underneath its icy crust and is supposedly in contact with the rocky mantle below, making the satellite particularly interesting from an astrobiological point of view. This is due to the peculiar composition of Europa which contains approximately 8% of water by mass.

In this paper we investigated the possible origin of the water content of Europa. We propose that Europa could have formed just inside the water snowline from drifting pebbles whose water ice content has been partially sublimated.

Phobos and Deimos origin of the martian moons

Reconciling the orbital and physical properties of the Martian moons

T. Ronnet, P. Vernazza, O. Mousis, B. Brugger, P. Beck, B. Devouard, O. Witasse, F. Cipriani 2016, ApJ.

The origin of Phobos and Deimos, the two small moons orbiting about Mars, is a long standing puzzle. Their physical properties make them resemble small primitive asteroids that could have been gravitationally captured by Mars. However, their nearly circular and coplanar orbits are hardly reconcilable with  a capture event.

Here we show that the formation of Phobos and Deimos following a giant impact on Mars allows to account for their spectral characteristics while it has been shown that it would also account for their orbital properties.

More publications

A. Luspay-Kuti and 12 co-authors (incl. T. Ronnet). Origin of Molecular Oxygen in Comets: Current Knowledge and Perspectives, SSRv 2018, Vol. 214, 115.
 

O. Mousis, T. Ronnet, J. I. Lunine, A. Luspay-Kuti, K. E. Mandt, G. Danger, F. Pauzat, Y. Ellinger, P. Wurz, P. Vernazza, L. Le Sergeant d’Hendecourt. Noble Gas Abundance Ratios Indicate the Agglomeration of 67P/Churyumov─Gerasimenko from Warmed-up Ice, ApJL 2018, Vol. 865, 11.
 

A. Bouquet and 8 co-authors (incl. T. Ronnet). Limits on the Contribution of Endogenic Radiolysis to the Presence of Molecular Oxygen in Comet 67P/Churyumov─Gerasimenko, ApJ 2018, Vol. 864, 9.

 

O. Mousis, T. Ronnet, J. I. Lunine, R. Maggiolo, P. Wurz, G. Danger, A. Bouquet. Synthesis of molecular oxygen via irradiation of ice grains in the protosolar nebula, ApJ 2018, Vol. 858, 66.

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O. Mousis and 55 co-authors (incl. T. Ronnet). Scientific rationale for Uranus and Neptune in situ explorations, P&SS 2017, Vol. 155, 12.

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O. Mousis, O. Ozgurel, J. I. Lunine, A. Luspay-Kutti, T. Ronnet, F. Pauzat, A. Markovits, Y. Ellinger. Stability of sulphur dimers (S2) in cometary ices, ApJ 2017, Vol. 835, 134.

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O. Mousis, T. Ronnet, B. Brugger, O. Ozgurel, F. Pauzat, Y. Ellinger, R. Maggiolo, P. Wurz, P. Vernazza, J. I. Lunine, A. Luspay-Kutti, K. E. Mandt, K. Altwegg, A. Bieler, A. Markovits, M. Rubin. Origin of molecular oxygen in Comet 67P/Churyumov-Gerasimenko, ApJL 2016, Vol. 823, L41.

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