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understanding its internal structure. Interpreting these geophysical data to model planetary structure and dynamics depends on understanding the physical properties of materials under relevant pressure and
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organic molecules in astrophysical environments—from cold interstellar ices to the early stages of planetary systems. The successful candidate will contribute to experimental studies simulating interstellar
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planetary geodynamics and habitability. Experience using piston cylinder and DAC presses, high-temperature and high-pressure experiments, numerical modeling, Zr isotopes, atomic-scale and micro-scale analyses
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Planetology (IRAP) in Toulouse, within the "Planetology, Environment and Space Plasmas," where interactions between researchers studying planetary surfaces and specialists in the space environment will help
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organic molecules in astrophysical environments—from cold interstellar ices to the early stages of planetary systems. The successful candidate will contribute to experimental studies simulating interstellar
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Sorbonne University, and is a partner of École des Ponts. Founded in 1968, the LMD studies climate and the environment for Earth and planetary atmospheres. This is an internationally renowned laboratory with
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73(1), 48. [7] Christensen et al (2001). A numerical dynamo benchmark. Physics of the Earth and Planetary Interiors 128(1-4), 25-34. - Get familiar with the literature regarding the core flow inverse