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9 Conclusion et intégration au Laboratoire Magmas et Vol-
cans

Depuis le début de ma thèse, je me suis intéressé aux grandes étapes d'évolution primitive des planètes et lunes du système solaire. J'ai travaillé plus particulièrement sur la relation entre les impacts météoritiques, l'évolution thermique des jeunes planètes et les premiers épisodes majeurs de différenciation. Cette thématique de recherche m'a naturellement amené à travailler sur la dynamique d'évolution du champ magnétique des planètes telluriques mais aussi à considérer des objets tels que les satellites de glace. Pour cela, j'ai développé et j'adapté des modèles numériques afin d'obtenir les échelles caractéristiques de temps, de longueur et de température propres à ces événements qui ont grandement conditionné la structure thermo-chimique actuelle des planètes.

<figure><img src="image_417.png" /></figure>

FIGURE 33 – Représentation schématique de l'évolution de la structure interne de la Terre depuis la fin de son accrétion jusqu'à la mise en place d'une tectonique des plaques moderne.

Au cours de mon parcours scientifique, j'ai utilisé des codes numériques (code d'analyse
de la déformation mécanique, code de convection, code de dynamo cinématique) et j'ai également modifié ces outils numériques afin de les adapter pour mieux comprendre comment évolue l'intérieur des jeunes planètes. J'ai ainsi transformé un code de convection 2D cartésien en un code de convection thermique axi-symétrique cylindrique puis en un code de convection thermo-chimique axi-symétrique sphérique afin de caractériser les conséquences d'un large impact météoristique sur une planète en croissance. J'ai modifié un code de convection thermique 3D sphérique pour inclure les effets de l'accrétion et de la différenciation des satellites de glace. Pour caractériser le refroidissement d'un océan magmatique impliquant tout le manteau terrestre j'ai développé une approche uni-dimensionnelle afin de pouvoir facilement implémenter des contraintes issues de la pétrologie expérimentale (courbes de fusion, adiabats, lois de viscosité...). Plus récemment, j'ai pris en main le logiciel COMSOL Multiphysics qui est un outil de modélisation en éléments finis permettant d'aborder différentes problématiques telles que les transferts thermiques, la mécanique des fluides et des solides ou les réactions chimiques. Il s'avère que cet outil est pertinent dans un laboratoire comme le LMV où les problématiques scientifiques sont très variées et où des progrès scientifiques majeurs nécessitants d'être envisagés d'un point de vue dynamique sont réguliers.

L'UMR 6524 Laboratoire Magmas et Volcans est une unité de recherche associée au CNRS. Ce laboratoire développe des programmes de recherche afin de comprendre l'ensemble des processus magmatiques et volcaniques, depuis la fusion dans le manteau terrestre jusqu'à l'éruption en surface en utilisant les méthodes et les outils les plus performants de différentes disciplines de la Pétrologie, de la Géochimie et de la Volcanologie et en s'appuyant sur un parc important d'appareillages expérimentaux et de caractérisations chimiques et physiques des roches et des minéraux. Mon arrivée au LMV en 2014 a permis d'apporter de nouvelles compétences en termes de modélisation numérique à ce laboratoire, en accord avec les évaluations AERES et HCERES qui avaient explicitement souligné le besoin du laboratoire en terme de modélisation géodynamique en complément, notamment, des approches transverses en pétrologie et géochimie isotopique sur les thématiques de la Terre interne et de l'origine du volcanisme.

Cette activité de recherche s'insère dans la thématique transverse «Terre primitive» du laboratoire (j'en suis l'animateur depuis 2022), et dont le but est de comprendre et caractériser les mécanismes géodynamiques, la structure interne et les signaux géochimiques des objets de la Terre primitive. Me concernant, ce laboratoire me permet de bénéficier d'expertises dans plusieurs domaines complémentaires, en particulier en géochimie et en pétrologie expérimentale qui apportent tous deux des contraintes majeures sur la séquence d'événements et les conditions dans lesquelles les processus d'accrétion et de différenciation planétaires se sont déroulées. Ainsi, ce projet est un élément charnière entre les membres de l'équipe Pétrologie (D. Andrault, A. Bouhifd, G. Manthilake) et ceux de l'équipe Géochimie dont plusieurs membres sont impliqués depuis longtemps dans l'analyse et la datation des éléments géochimiques traceurs des évènements terrestres primitifs (M. Boyet, M. Garçon, M. Guitreau). Ce projet permet ainsi de donner une autre dimension à ces deux équipes en apportant des contraintes sur la dynamique, les forces, la physique des mouvements que la géochimie et la
pétrologie expérimentale ne peuvent pas traiter.

Les moyens nécessaires pour mener à bien mon activité de recherche sont des instruments de calcul puissants permettant de lancer des codes numériques résolvant les équations de la dynamique des fluides que j’ai déjà développés ou que je souhaite adapter au quotidien. Ces instruments sont déjà présents au sein de l’UMR puisque celle-ci possède des moyens de calcul aux niveaux local (clusters), régional (Centre de Calcul Intensif Auvergrid) et bénéficie d’accès aux centres nationaux (le Centre Informatique National de l’Enseignement Supérieur et Institut du Développement et des Ressources en Informatique Scientifique).

Les neuf années que j’ai passées au Laboratoire Magmas et Volcans m’ont permis de voir quels étaient mes besoins pour aller plus loin dans mon activité de recherche mais aussi pour développer la modélisation numérique dans ce laboratoire. Tout d’abord, mon expérience d’encadrement des thèses de Baraa Qaddah (2017-2020) et de Tristan Engels (2021-2024) montrent qu’il est possible d’attirer et de conserver des étudiants motivés pour des travaux liés à la dynamique interne de le Terre Primitive alors que l’offre de formation attire plutôt des étudiants en volcanologie. Les étudiants formés à l’Université Clermont-Auvergne dans le parcours Magmas et Volcans sont sensibilisés à la mécanique des fluides, aux questions liées à la Terre primitive et à la dynamique de la Terre interne. J’envisage prochainement de déposer à l’École Doctorale un sujet lié aux effets de marées sur le refroidissement de la Terre primitive.

De plus, ces neuf années ont été jalonnées de projets et de publications avec des collègues qui souhaitaient renforcer leurs conclusions ou aller au-delà de leur expertise en s’appuyant sur des modèles numériques. Ainsi aujourd’hui il est courant que je développe des modèles avec des géochimistes (M. Guitreau, M. Boyet) et avec des spécialistes de la pétrologie expérimentale (D. Andrault, A. Bouhifd, G. Manthilake). Ces collaborations n’ont pas pour autant limité mes collaborations avec des chercheurs d’autres laboratoires que ce soit en France (M. Le Bars, G. Tobie, H. Samuel, P. Auclair-Desrotour) ou à l’étranger (J. Arkani-Hamed, S. Marchi).

Enfin, les collaborations récentes avec mes collègues pétrologues, géochimistes mais aussi volcanologues m’ont montré à quel point il fallait être réactif en terme de développement numérique afin de pouvoir apporter regard différent sur leurs résultats expérimentaux. Par exemple, je développe actuellement des modèles numériques en collaboration avec O. Roche afin de calibrer un dispositif expérimental permettant de caractériser la dynamique d’une chambre magmatique. Il s’agit notamment de caractériser l’effet d’injection de magmas sur la fusion et la remobilisation du matériel fondu pré-éxistant. Pour cela, O. Roche et moi avons travaillé sur le dimensionnement d’une expérience en laboratoire impliquant des matériaux analogues (liquides, volatils, particules). Notre collaboration a permis de designer au mieux le dispositif expérimental de cette étude. Mais pour développer ces modèles numériques, nous avons besoin de considérer des géométries et des rhéologies complexes et de tels modèles ne peuvent être développés que sur des échelles de temps courtes. Ainsi il semble qu’un outil tel que COMSOL Multiphysics soit particulièrement adapté dans ce laboratoire. Et au vu du nombre croissant des sollicitations, il serait à l’avenir intéressant d’avoir au LMV un Ingénieur
dédié au développement de tels modèles.
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pacts and consequences for mantle convection. Journal of Geophysical Research (Planets)
114, E02001.

Wiechert, U., Halliday, A. N., Lee, D.-C., Snyder, G. A., Taylor, L. A., Rumble, D., Oct. 2001.
Oxygen Isotopes and the Moon-Forming Giant Impact. Science 294, 345–348.

Willbold, M., Elliott, T., Moorbath, S., Sep. 2011. The tungsten isotopic composition of the Earth's mantle before the terminal bombardment. Nature 477 (7363), 195–198.

Williams, G. E., Jan. 2000. Geological constraints on the Precambrian history of Earth's rota-
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Williams, J., Nimmo, F., 2004. Thermal evolution of the Martian core : Implications for an early dynamo. Geology 32.

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10 Annexes
10.1 Annexe 1 : Curriculum Vitae
Julien MONTEUX

Chargé de Recherche CNRS Classe Normale
Qualifié en sections 35 et 36
Laboratoire Magmas et Volcans
Campus universitaire des Cézeaux,
6 Avenue Blaise Pascal,
63170 Aubière

RENSEIGNEMENT PERSONNELS :

Date de naissance : 8 Juin 1982

Lieu de naissance : Saint-Etienne

Nationalité : Française

Statut marital : Marié, 3 enfants

INTERÊTS SCIENTIFIQUES :

- Modélisation numérique de la dynamique des fluides: convection thermo-chimique pour différentes géométries.

- Impacts météoritiques et différenciation des planètes

- Initiation/évolution du champs magnétique des planètes

- Accrétion et évolution thermo-chimique des planètes

FORMATION :

Septembre 2000-Juin 2002

Classe Préparatoire aux Grandes Ecoles, option Biologie Chimie
Physique et Sciences de la Terre.

Lycée C. Fauriel, Saint-Etienne, France

Septembre 2002-Juin 2003

Licence en Géosciences - Géophysique,
Ecole Normale Supérieure de Lyon, Université Lyon 1, France

Septembre 2003-Juin 2005

Master en Géosciences - Géophysique,
Physique Chimie de la Terre et de Planètes
Ecole Normale Supérieure de Lyon, Université Lyon 1, France

Octobre 2005-Janvier 2009

Doctorat en Sciences de la Terre, Laboratoire des Sciences de la Terre,
École Normale Supérieure de Lyon, Université Lyon 1, France

EXPÉRIENCES EN RECHERCHE:

Janvier 2003-Juillet 2003

Stage de Licence : Évolution du champ de gravité terrestre et observation du
rebond post-glaciaire.

Encadrants : F. Chambat, Laboratoire des Sciences de la Terre, École Normale Supérieure de Lyon, CNRS.
Janvier 2004-Juillet 2004

**Stage de M.2R.** : Modélisation mécanique de la déformation de la croûte océanique sous les volcans d'Hawaii.

Encadrants : J.-L. Got et R. Hassani (Laboratoire de Géophysique Interne et de Tectonophysique de Chambéry, Université de Savoie.)

Octobre 2005-Janvier 2009

**Thèse** : Modélisation numérique de la formation du noyau terrestre

**Financement Bourse M.R.T. (allocataire moniteur)**

Encadrants : N. Coltice, Y. Ricard et F. Dubuffet, (Laboratoire des Sciences de la Terre, Université de Lyon, École Normale Supérieure de Lyon, Université Claude Bernard Lyon 1, CNRS).

Février 2009-Septembre 2010

**Post-Doctorat** : Modélisation numérique de l'initiation du champ magnétique des objets du système solaire.

**Financement Bourse Lavoisier**

Encadrants : M. Jellinek et C. Johnson (Earth and Ocean Sciences Laboratory, University of British Columbia, Vancouver, Canada).

Septembre 2010-Avril 2014

**Jeune Chercheur** : Accrétion et Différenciation des Satellites de Glace, Évolution des dynamos planétaires.

**Financement A.N.R. Retour Post-doc (projet Accrétis)**

Collaborateurs : G. Tobie, G. Choblet, H. Amit, B. Langlais (Laboratoire de Planétologie et de Géodynamique de Nantes).

Mai 2014- Octobre 2016

**Jeune Chercheur** : Évolution thermo-chimique d'un océan magmatique

**Financement A.N.R. Oxydeep + Auvergne Fellowship**

Collaborateurs : Denis Andrault, Ali Bouhifd (Laboratoire Magmas et Volcans de Clermont-Ferrand), Henri Samuel (IRAP, Toulouse).

Depuis Octobre 2016

**Chargé de Recherche CNRS CN** : Accrétion et différenciation

de la Terre primitive ; Évolution thermochimique jusqu'à aujourd'hui.

Collaborateurs : Denis Andrault, Ali Bouhifd, Geeth Manthilake, Maud Boyet (Laboratoire Magmas et Volcans de Clermont-Ferrand), Henri Samuel (IRAP, Toulouse), Gabriel Tobie (LPG, Nantes), Michael Le Bars (IRPHE, Marseille).

## PRINCIPAUX FINANCEMENTS

2023 Origines/INSU : Deep Earth-MOon Tidal Coupling: a signature in the geochemical record and in the current orbital configuration? 11 000 €

2021 LABEX ClerVolc : Formation des atmosphères primitives des planètes : Le comportement des volatils (C, H, N, O et S) durant les impacts, 108 000 €

2020 PNP/INSU : Modélisation du rôle des impacts sur la composition en éléments volatils de la Lune, 5 500 €
2020 UCA-WOW Mobilité sortante : *Modélisation du rôle des impacts sur la composition en éléments volatils de la Lune*, 5541 €

2020 LABEX ClerVolc : *Modélisation du rôle des impacts sur la composition en éléments volatils de la Lune*, 8 200 €

2017 PNP/INSU : Modélisation numérique de l'équilibration thermochimique pendant la ségrégation du fer dans un océan magmatique, 7 000 €

2017 LABEX ClerVolc : *Plate-forme de modélisation numérique multi-utilisateurs COMSOL Multiphysics*, 29 000 €

2015 Auvergne Fellowship, LMV - 2 year-project
*Évolution thermo-chimique d'un océan magmatique*, 100 000 €

2010 ANR Retour Post-doc Fellowship (PI), LPG Nantes, France –
Accrétion et évolution thermique des satellites de glace
3 year-project, 154 000 €
20 projects funded in France for 150 applications
https://anr.fr/Project-ANR-10-PDOC-0001

2009 Fellowship of excellence Lavoisier (PI) UBC, Canada – 1 year-project, 15 000 €
1980 laureates for 5,500 candidates in 2009.

## ENCADREMENT :

2016-2017 1 post-doctorant : **Vincent Clési** (LMV, France)
*Numerical modelling of core mantle separation* (2 publications)

2016-2023 3 Étudiants en thèse
* **Tristan Engels** (2021-2024) (LMV France)
* *Formation des atmosphères primitives des planètes : Le comportement des éléments volatils (C, H, N, O et S) durant les impacts*

* **Remy Pierru** (2018-2021) (LMV France)
* *Deep mantle melting and consequences for the Early Earth dynamics*

* **Baraa Qaddah** (2017-2020) (LMV France)
* *Numerical modelling of the dynamics and thermal evolution of a metal drop in free fall in a viscous medium* (4 publications)

2012-2023 3 Étudiants en Master
* **Tristan Engels** (LMV, France), **Laura Clodoré** (LMV-LPGN), **Nadejda Marounina** (LPG, Nantes)

2020-2024 3 Étudiants en Licence
* **Anaëlle Antunes** (LPG, Nantes), **Yoan Luzy** (LMV, France) et **Tristan Bablin** (LMV, France)
## ENSEIGNEMENT

2014 Université Clermont-Auvergne, France
CM : Modélisation numérique de la dynamique interne de la Terre (3h/an)
CM et TD: Petrologie (Licence, 30h)

2010 – 2014 Université de Nantes, France
TD et CM (Master, 80h)

2009 – 2010 University of British Columbia, Vancouver, Canada
Responsable administratif du cours "Natural disaster" (1100 élèves)

2005 – 2009 Université Claude Bernard Lyon 1, France
TD et CM (Licence+Master, Monitorat + ½ ATER : 290h)

## ORGANISATION DE CONGRÈS SCIENTIFIQUE

2018 Membre du comité d'organisation de l' EMPG 16 (Clermont-Ferrand, France):
International Symposium on Experimental Mineralogy, Petrology and Geochemistry
(212 participants).

## ANIMATION ET MANAGEMENT DE LA RECHERCHE

2022- Membre du conseil scientifique du Programme National de Planétologie (domaines A.A. et TS de l'INSU)

2022- Responsable de l'axe transverse « Géodynamique de la Terre
Primitive » au Laboratoire Magmas et Volcans

2022- Responsable du thème «Origin of Volcanoes and of the Earth» du Labex Clervolc.

2017- Membre élu du conseil du Laboratoire Magmas et Volcans

2017- 2023 Membre de la Cellule Communication du Laboratoire

2017- 2023 Correspondant de la Commission Diffusion de la Culture Scientifique, Technique et Industrielle (DCSTI) au sein de l'Université Clermont-Auvergne

2017- 2023 Membre de la commission «Modélisation et concepts connexes» à l'Université Clermont-Auvergne

## DIFFUSION SCIENTIFIQUE

* Membre du conseil scientifique (CS) et Participation au festival Nuées Ardentes

* Membre du CS et Participation au festival Rencontres Montagnes et Sciences

* Membre du CS d'Astusciences

* Organisation de la Fête de la Science au Laboratoire Magmas et Volcans

## ACTIVITIES EDITORIALES

2005 – present Reviewer pour Nature, Nature Geosciences, Earth and Planetary Science Letters, Physics of the Earth and Planetary Interiors, Icarus, Journal of Geophysical Research, Monthly Notices of the Royal Astronomical Society, Planetary and Space Science.
10.2 Annexe 2 : Valorisation des travaux
LISTE DES PUBLICATIONS

•[35] Bouhifd M.A., M. Boyet, N. Bolfan-Casanova, G. Manthilake, **J. Monteux**, M. Roskosz, F. Gaillard and D. Andrault, Water budget on Earth and its early reservoirs: Bulk Silicate Earth and Core, subm. to Geochem. Persp. Lett.

•[34] Engels. T., **Monteux J.**, Boyet M., Bouhifd M.A., Large impacts and their contribution on the volatile budget of the Early Moon. In revision for Icarus

•[33] **Monteux J.**, Qaddah B., Andrault D., Conditions for segregation of a crystal-rich layer within a convective magma ocean. In revision for J. Geophys Res.

•[32] Pierru R., Andrault D., Manthilake G., **Monteux J.**, Devidal J.L., Guignot N., King A., Henry L. Deep mantle origin of large igneous provinces and komatiites, Accepted in Science Advances.

•[31] Freitas D., **Monteux J.**, Andrault D., Manthilake G., Mathieu A., Schiavi F., Cluzel N. (2021). Thermal conductivities of solid and molten silicates: Implications for dynamos in mercury-like proto-planets. Physics of the Earth and Planetary Interiors vol.312, p.106655

•[30] B. Qaddah, **J. Monteux**, M. Le Bars, Thermal evolution of a metal drop falling in a less dense, more viscous fluid, (2020) Phys. Rev. Fluids, 5, 053801.

•[29] V. Clési, **J. Monteux**, B. Qaddah, M. Le Bars, J.B. Wacheul, M. A. Bouhifd, Dynamics of core-mantle separation: Influence of metal and silicate viscosity on the chemical equilibrium, (2020) Phys. Earth Planet. Int. Volume 306, 106547.

•[28] **Monteux J.**, Andrault D., Guitreau M., Samuel H., Demouchy S. (2020). A mushy Earth's mantle for more than 500 Myr after the magma ocean solidification. Geophys. J. Int. vol.221, p.1165-1181.

•[27] Frossard P., Boyet M., Bouvier A., Hammouda T., **Monteux J.** (2019). Evidence for anorthositic crust formed on an inner solar system planetesimal. *Geochemical Perspectives Letters* vol.11, p.28-32, DOI:10.7185/geochemlet.1921.

•[26] Manthilake G., Chantel J., **Monteux J.**, Andrault D., Bouhifd A., Bolfan-Casanova N., Boulard E., Guignot N., King A., Itie J.P. (2019). Thermal Conductivity of FeS and Its Implications for Mercury's Long-Sustaining Magnetic Field. *Journal of Geophysical Research* - *Planets* vol.124, DOI:10.1029/2019JE005979.

•[25] **Monteux J.**, Arkani-Hamed J. (2019). Shock wave propagation in layered planetary interiors: Revisited. *Icarus* vol.331, p.238-256, DOI:10.1016/j.icarus.2019.05.016.

•[24] Qaddah B., **Monteux J.**, Clesi V., Bouhifd A., Le Bars M. (2019). Dynamics and stability of an iron drop falling in a magma ocean. *Physics of the Earth and Planetary Interiors* vol.289, p.75-89, DOI:10.1016/j.pepi.2019.02.006.

•[23] Andrault D., Pesce G., Manthilake G., **Monteux J.**, Bolfan-Casanova N., Chantel J., Novella D., Guignot N., King A., Itié J.P., Hennet L. (2018). Deep and persistent melt layer in the Archaean mantle. *Nature Geoscience* DOI:10.1038/s41561-017-0053-9.
•[22] **Monteux J.**, Golabek G.J., Rubie D.C., Tobie G., Young E.D. (2018). Water and the interior structure of terrestrial planets and icy bodies. Space Science Reviews. ISSN: 0038-6308 (Print) 1572-9672 (Online).

•[21] Andrault D., Bolfan-Casanova N., Bouhifd A., Boujibar A., Garbarino G., Manthilake G., Mezouar M., **Monteux J.**, Parisiades P., Pesce G. (2017). Toward a coherent model for the melting behavior of the deep Earth's mantle. *Physics of the Earth and Planetary Interiors* vol.265, p.67-81, DOI:10.1016/j.pepi.2017.02.009.

•[20] Bouhifd A., Clesi V., Boujibar A., Bolfan-Casanova N., Cartier C., Hammouda T., Boyet M., Manthilake G., **Monteux J.**, Andrault D. (2017). Silicate melts during Earth's core formation. *Chemical Geology* vol.461, p.128 - 139, DOI:10.1016/j.chemgeo.2016.12.035.

•[19] Andrault D., **Monteux J.**, LeBars M., Samuel H. (2016). The deep Earth may not be cooling down. *Earth and Planetary Science Letters* vol.443, p.195-203, DOI:10.1016/j.epsl.2016.03.020.

•[18] Guillaume B., Pochat S., **Monteux J.**, Husson L., Choblet G. (2016). Can eustatic charts go beyond first order? Insights from the Permian–Triassic. *Lithosphere* DOI:10.1130/L523.1.

•[17] **Monteux J.**, Andrault D., Samuel H. (2016). On the cooling of a deep terrestrial magma ocean. *Earth and Planetary Science Letters* vol.448, p.140-149, DOI:10.1016/j.epsl.2016.05.010.

•[16] **Monteux J.** Arkani-Hamed J. (2016). Scaling Laws of Impact Induced Shock Pressure and Particle Velocity in Planetary Mantle. *Icarus* vol.264, p.246-256, DOI:10.1016/j.icarus.2015.09.040.

•[15] **Monteux J.**, Collins G.S., Tobie G., Choblet G. (2016). Consequences of large impacts on Enceladus' core shape. *Icarus* vol.264, p.300-310, DOI:10.1016/j.icarus.2015.09.034.

•[14] Amit H., Choblet, G., Olson P., **Monteux J.**, Deschamps F., Langlais B., Tobie G. (2015). Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamos. *Progress in Earth and Planetary Science* p.2-26, DOI:10.1186/s40645-015-0056-3.

•[13] Boujibar A., Andrault D., Bolfan-Casanova N., Bouhifd A., **Monteux J.** (2015). Cosmochemical fractionation by collisional erosion during the Earth's accretion. *Nature Communications* vol.6, p.8295, DOI:10.1038/ncomms9295 | www.nature.com/naturecommunications.

•[12] Marounina N., Tobie G., Carpy, **Monteux J.**, Charnay B., Grasset O. (2015). Evolution of Titan's atmosphere during the Late Heavy Bombardment. *Icarus* vol.257, p.324-335, DOI:10.1016/j.icarus.2015.05.011.

•[11] **Monteux J.**, Amit H., Choblet G., Langlais B., Tobie G. (2015). Giant impacts, heterogeneous mantle heating and a past hemispheric dynamo on Mars. *Physics of the Earth and Planetary Interiors* vol.240, p.114-124, DOI:10.1016/j.pepi.2014.12.005.
•[10] Wacheul, J.B., Le Bars, M., **Monteux, J.**, Aurnou, J.M., (2014) Laboratory experiments on the breakup of liquid metal diapirs, Earth and Planet. Sci. Lett, Volume 403, Pages 236-245

•[9] **Monteux, J.**, G., Tobie, G., Choblet, M., Le Feuvre, (2014) Can large icy Moons accrete undifferentiated, Icarus, Volume 237, 15 July 2014, Pages 377-387

•[8] **Monteux, J.**, J., Arkani-Hamed (2014), Consequences of giant impacts in early Mars: Core merging and Martian dynamo evolution, J. Geophys. Res. (Planets), Volume 119, Issue 3, pages 480–505

•[7] Tobie, G., J.I. Lunine, **J. Monteux**, O. Mousis, F. Nimmo (2013), The Origin and Evolution of Titan, Titan: Surface, Atmosphere and Magnetosphere edited by I. Mueller-Wodarg, C. Griffith, T. Cravens and E. Lellouch for Cambridge University Press.

•[6] **Monteux, J.**, M. Jellinek, C. J., Johnson, (2013) Dynamics of core merging after a martian mega-impact, Icarus, 226, Issue 1, Pages 20–32.

•[5] **Monteux, J.**, N. Schaeffer, H. Amit, P. Cardin, (2012) Can a sinking metallic diapir generate a dynamo? J. Geophys. Res. (Planets), 117, E10005, 14 PP.,doi:10.1029/2012JE004075

•[4] **Monteux, J.**, M. Jellinek, C. J., Johnson (2011), Why might planets and moons have early dynamos?, Earth and Planet. Sci. Lett., 310, 349-359.

•[3] **Monteux, J.**, Y. Ricard, N. Coltice, F. Dubuffet, M. Ulvrova (2009), A model of Metal-Silicate separation on Growing Planets, Earth and Planet. Sci. Lett., 287,353-362.

•[2] Got, J.L., V. Monteiller, **J. Monteux**, R. Hassani, P. Okubo (2008), Deformation and rupture of the oceanic crust may control growth of hawaiian volcanoes, Nature, 451, 453-456.

•[1] **Monteux, J.**, N. Coltice, F. Dubuffet, Y. Ricard (2007), Thermo-mechanical adjustment after impacts during planetary growth, Geophys. Res. Lett, 34, L24201.

## CHAPITRES D'OUVRAGES:

* Monteux J., Andrault, D., (2023). Dynamique et évolution thermique du manteau terrestre primitif. In Dynamique du manteau terrestre (resp. J. Monteux). Encyclopédie ISTE. Thème Terre interne (ed. N. Bolfan-Casanova).

* Monteux J., Golabek G.J., Rubie D.C., Tobie G., Young E.D. (2018). Water and the interior structure of terrestrial planets and icy bodies. In The Delivery of Water to Protoplanets, Planets and Satellites, Space Science Series of ISSI. ISSN: 0038-6308 (Print) 1572-9672 (Online).

* Andrault D., Bolfan-Casanova N., Bouhifd A., Boujibar A., Boyet M., Cartier C., Clesi V., Doucelance R., Hammouda T., Laubier M., Manthilake G., Marin-Carbonne J., Martin H., Moine B., Monteux J., Moyen J.F., Paquette J.L. (2017). Environnement de la Terre primitive: Comment construire une planète habitable ? Groupe de Recherche : "Mécanismes géodynamiques de la Terre primitive". Revue d'Auvergne vol.262-263, p.7-40.
* Tobie, G., J.I. Lunine, J. Monteux, O. Mousis, F. Nimmo (2013), The Origin and Evolution of Titan, Titan: Surface, Atmosphere and Magnetosphere edited by I. Mueller-Wodarg, C. Griffith, T. Cravens and E. Lellouch for Cambridge University Press.
PARTICIPATION À DES CONGRÈS SCIENTIFIQUES INTERNATIONAUX

* [46] Andrault D., **Monteux J.** (2023). Thermochemical modelling of chemical segregation in a crystallizing magma ocean. Goldschmidt conference, Lyon, France (2023).

* [45] **Monteux J.**, Qaddah B., Andrault D. (2023). Conditions for segregation of a crystal-rich layer within a convective magma ocean. Goldschmidt conference, Lyon, France (2023).

* [44] Engels T., **Monteux J.**, Boyet, M., Bouhifd A. (2023). Large impacts and their contribution on the volatile budget of the Early Moon. Goldschmidt conference, Lyon, France (2023).

* [43] Engels T., **Monteux J.**, Bouhifd A. (2022). Large impacts and their contribution on the volatile budget of the Early Moon. Programme National de Planétologie, Lyon (2022).

* [42] **Monteux J.**, Qaddah B., Andrault D. (2022). Stability of a thin mushy layer within a convecting magma ocean. Programme National de Planétologie, Lyon (2022).

* [41] Andrault D., **Monteux J.**, Pison L., Mathieu A. (2022). New measurements of Fe thermal conductivity and implications for the thermal history of the Earth's core. Programme National de Planétologie, Lyon (2022).

* [40] Frossard P., Boyet M., Bouvier A., Hammouda T., **Monteux J.** (2020), The diversity of early planetesimals crusts: Insights from NWA 7325/8486 and NWA 11119, École d'été des Houches.

* [39] Pierru R., Andrault D., Manthilake G., **Monteux J.**, Devidal J.L., Guignot N., King A. Mantle Origin of the Large Igneous Provinces. AGU fall meeting, New Orleans, USA, (2021).

* [38] **Monteux J.**, Qaddah B., Andrault D. (2021). Stability of a crystallizing layer within a (convecting) magma ocean. AGU fall meeting, New Orleans, USA, (2021).

* [37] Andrault D., Pison L., **Monteux J.**, Mathieu A., Thermal history of the Earth's core: new measurements of Fe thermal conductivity. AGU fall meeting, New Orleans, USA, (2021).

* [36] **Monteux J.**, Qaddah B., Andrault D. (2021). Stability of a crystallizing layer within a (convecting) magma ocean. Goldschmidt conference, Lyon, France (2021).

* [35] Frossard P., Boyet M., Bouvier A., Hammouda T., **Monteux J.** (2019). Magma cean-dervied anorthositc crust on early (<5 Ma) planetesimals. 50th Lunar and Planetary Conference, Houston, USA.

* [34] **Monteux, J.**, Andrault, D., Guitreau, M., Samuel, H., Demouchy, S., The influence of the Earth's early mantle viscosity on its cooling dynamics, EPSC-DPS Joint Meeting 2019.

* [33] Manthilake G., Chantel J., Andrault D., **Monteux J.**, Bouhifd A., Bolfan-Casanova N., Boulard E., Guignot N., King A., Itie J.P. (2018). Electrical conductivity of Fe–S alloys at high pressure and high temperature: Implications for Mercury’s weak and long-lived magnetic field. EMPG XVI conference abstract, Clermont-Ferrand, 17-21 juin 2018.
* [32] **Monteux J.**, Andrault D., Samuel H. (2018). On the cooling of a deep mushy mantle. EMPG XVI Conference abstract, Clermont-Ferrand, 17-21 juin 2018.

* [31] Qaddah B., **Monteux J.**, Le Bars M., Clesi V., Bouhifd A. (2018). The breakup of liquid iron diapirs within the magma ocean. EMPG XVI Conference abstract, Clermont-Ferrand, 17-21 juin 2018.

* [30] Qaddah B., **Monteux J.**, Le Bars M., Clesi V., Bouhifd A. (2018). The breakup of liquid iron diapirs within the magma ocean. Study of the Earth Deep Interior (SEDI 2018), Edmonton (Canada), 8-13 Jul 2018.

* [29] Arkani-Hamed J., **Monteux J.** (2017). Shock Wave Propagation in Layered Planetary Interiors: Revisited. AGU Fall Meeting abstract, New Orleans, USA.

* [28] **Monteux J.**, Arkani-Hamed J. (2017). Shock Wave Propagation in Layered Planetary Interiors: Revisited. AGU Fall meeting, New Orleans.

* [27] Samuel H., Michaut C., Baratoux D., **Monteux J.**, Andrault D., Kurita K. (2017). The Early Thermal Evolution and Delamination of Mars' Crust. Goldschmidt, Paris.

* [26] Drummond Mc.G., Thieulot C., **Monteux J.** (2016). The effect of giant impactors on the magnetic field energy of an early Martian dynamo. EGU General Assembly 2016.

* [25] Guillaume B., **Monteux J.**, Pochat S., Husson L., Choblet G. (2016). Can eustatic charts go beyond first-order? Insights from the Permo-Triassic. EGU General Assembly 2016.

* [24] **Monteux J.**, Andrault D., Samuel H. (2016). On the cooling of a deep terrestrial magma ocean. SEDI, Nantes, 24-29 Juillet 2016.

* [23] Andrault D., **Monteux J.**, Le Bars M., Samuel H. (2015). A steady thermal state for the Earth's interior. AGU Fall Meeting, San Francisco, 14-18 décembre 2015.

* [22] **Monteux J.**, Amit H., Arkani-Hamed J., Choblet G., Langlais B., Tobie G., Johnson C.L., Jellinek M. (2015). Consequences of Giant Impacts on the Martian dynamo. AGU Fall Meeting, San Francisco, 14-18 décembre 2015.

* [21] **Monteux J.**, Amit H., Choblet G., Langlais B., Tobie G. (2015). Giant impacts, heterogeneous mantle heating and a past hemispheric dynamo on Mars. vol.17, p.EGU2015-1723-2, Geophysical Research Abstracts, EGU General Assembly 2015.

* [20] **Monteux J.**, Andrault D., Samuel H. (2015). On the cooling of a deep terrestrial magma ocean. European Planetary Science Congress 2015, Nantes, France, 27 September - 2 October, 2015.

* [19] **Monteux J.**, Andrault D., Samuel H. (2015). On the cooling of a deep terrestrial magma ocean. AGU Fall Meeting, San Francisco, 14-18 décembre 2015.

* [18] **Monteux J.**, Arkani-Hamed J. (2015). Scaling Law of Impact Induced Shock Pressure in Planetary Mantle. 46th Lunar and Planetary Science Conference (2015).

* [17] **Monteux J.**, Arkani-Hamed J. (2015). Scaling Law of Impact Induced Shock Pressure
in Planetary Mantle. vol.17, p.EGU2015-3785, Geophysical Research Abstracts, EGU General Assembly 2015.

[16] **Monteux J.**, Collins G. S., Tobie G., Choblet G. (2015). Consequences of large impacts on Enceladus' core shape. European Planetary Science Congress 2015, Nantes, France, 27 September - 2 October, 2015.

[15] Pesce G., Manthilake G., Andrault D., **Monteux J.**, Bolfan-Casanova N., Novella D., Guignot N., Chantel J. (2015). On the cooling of a deep terrestrial magma ocean: Experimental perspective. AGU Fall Meeting.

[14] Pesce, G., Andrault D., Manthilake G., **Monteux J.**, Bolfan-Casanova N., Novella D., Guignot N., Chantel J. (2015). On the cooling of a deep terrestrial magma ocean: Experimental perspectives. AGU Fall Meeting, San Francisco, 14-18 décembre 2015.

[13] **Monteux, J.**, Arkani-Hamed (2014) Thermal Consequences of Giant Impacts and Core Merging in Early Mars, Accrete Workshop, Nice (France).

[1] 2 Amit, H., Choblet, G., Olson, P., **Monteux, J.**, Deschamps, F., Langlais. B, Tobie, G. (2014) Planetary dynamos features driven by exotic models of core-mantle boundary heat flux, SEDI, Kanagawa (Japon)

[11] Wacheul, J.B., Le Bars, M., Aurnou, J.M., **Monteux, J.** (2013), Experiments on the stability of metal diapirs, American Geophysical Union, Fall Meeting 2013.

[10] **Monteux, J.**, G. Tobie, G. Choblet, M. Le Feuvre (2012), Can Large Icy Moons Accrete Undifferentiated, American Geophysical Union, Fall Meeting 2012.

[9] **Monteux, J.**, M. LeBars, O. Aubert (2012), Influence of the viscosity contrast on the metal diapir breakup in primitive magma oceans, American Geophysical Union, Fall Meeting 2012.

[8] **Monteux, J.**, N. Schaeffer, H. Amit, P. Cardin (2012), Can a sinking diapir generate a dynamo?, American Geophysical Union, Fall Meeting 2012.

[7] **Monteux, J.**, G. Tobie, G. Choblet, M. Le Feuvre (2012), Can Large Icy Moons Accrete Undifferentiated, EPSC, 2012.

[6] **Monteux, J.**, N. Schaeffer, H. Amit, P. Cardin (2011), Can a sinking diapir generate a dynamo?, EPSC-DPS, 2011.

[5] **Monteux, J.**, M. Jellinek, C.J. Johnson (2010), Why might planets and moons have early dynamos?, Lunar and Planet. Sci. Conf., 2010.

[4] **Monteux, J.**, M. Jellinek, C.J. Johnson (2009), Why might planets and moons have early dynamos?, American Geophysical Union, Fall Meeting 2009.

[3] **Monteux, J.**, N. Coltice, F. Dubuffet, Y. Ricard (2008), Thermo-mechanical adjustment after impacts during planetary growth, European Geosciences Union 2008.

[2] J.-L. Got, **J. Monteux**, V. Monteiller, R. Hassani, P. Okubo (2007), Better understanding of Hawaiian volcanoes through double-difference tomography and
mechanical modelling, European Geosciences Union 2007.

* [1] **Monteux, J.**, N. Coltice, F. Dubuffet, Y. Ricard (2006), Dynamics of magma ocean formation after large impacts, American Geophysical Union, Fall Meeting 2006, abstract#V11D-0609.
VALORISATION ET DIFFUSION SCIENTIFIQUE

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10.3 Annexe 3 : Publications dans d'autres thématiques

Got, J.L., V. Monteiller, **J. Monteux**, R. Hassani, P. Okubo (2008), *Deformation and rupture of the oceanic crust may control growth of hawaiian volcanoes*, Nature, 451, 453-456.
**LIEN HAL.**

Guillaume B., Pochat S., **Monteux J.**, Husson L., Choblet G. (2016). Can eustatic charts go beyond first order ? Insights from the Permian–Triassic. Lithosphere - DOI :10.1130/L523.1.
**LIEN HAL.**