16:45 to 18:45
Lecture

The isotopic dichotomy

Alessandro Morbidelli
Asteroids and their samples : meteorites - witnesses to the first phases of planetary formation
16:45 to 18:45
    Amphithéâtre Marguerite de Navarre, Site Marcelin Berthelot
    Open to all, subject to availability
    -

    Documents and media

    Speaker(s)

    Alessandro Morbidelli

    Professor at the Collège de France

    Events

    Lecture
    16:45 to 18:45
    Alessandro Morbidelli

    The asteroid belt
    Lecture
    16:45 to 18:45
    Alessandro Morbidelli

    Meteorites and where they come from
    Lecture
    17:00 to 18:00
    Alessandro Morbidelli

    Refractory inclusions
    Seminar
    18:00 to 19:00
    Adnan Ahmad

    Formation of protoplanetary disks and CAI transport mechanisms
    Lecture
    16:45 to 17:45
    Alessandro Morbidelli

    Chonders
    Seminar
    17:45 to 18:45
    Yves Marrocchi

    The story of solar system dust told by chondrules
    Lecture
    16:45 to 17:45
    Alessandro Morbidelli

    Planetesimal formation : constraints
    Seminar
    17:45 to 18:45
    Clara Maurel

    The paleomagnetism of meteorites : from the evolution of the protoplanetary disk to the i…
    Lecture
    16:45 to 18:45
    Alessandro Morbidelli

    The isotopic dichotomy
    Lecture
    16:45 to 18:45
    Alessandro Morbidelli

    Dust dynamics and planetesimal formation : theory vs. …
    Lecture
    17:00 to 18:00
    Alessandro Morbidelli

    A (partial) overview of the early evolution of the inner solar system
    Seminar
    18:00 to 19:00
    Sébastien Charnoz

    Out-of-balance condensation and oxidation in the Solar System
    Lecture
    16:45 to 18:45
    Alessandro Morbidelli

    Formation and evolution of the asteroid belt

    See also

    Seminar related to the lecture: Asteroids and their samples: meteorites - Witnesses to the first phases of planetary formation
    Alessandro Morbidelli, chair Planetary Formation: from Earth to Exoplanets
    Asteroids and their samples : meteorites - witnesses to the first phases of planetary formation