Astrochemistry and Origins

How to measure and visualize in 3D the composition and structure of a micrometric extraterrestrial grain without destroying it? Researchers from the "Astrochemistry and Origin" team of the IAS and from the SOLEIL synchrotron, in collaboration with two Japanese laboratories, have shown that this is possible. Coupling IR and X-ray micro-tomography the scientist analyzed samples from the asteroid Itokawa, collected by the Hayabusa probe (JAXA).

Although there are evidences of relationships between the most primitive bodies of the solar system and differentiated planetary bodies with a metallic core, no sample has been found up to now that bears information on the onset of planetary differentiation. Researchers have recently described a volcanic rock produced by extremely limited partial melting of a parent body chemically similar to the most primitive meteorites (carbonaceous chondrites) and crystallized upon ascent toward the surface of the body. This sample proves that some carbonaceous bodies from the outer solar system are partially differentiated and is the missing link in a continuum between comets and iron meteorites from metallic planetary cores.