ISMO

Institut des Sciences Moléculaires d'Orsay


Partenaires

CNRS UPS




lundi 22 avril


Mise à jour
jeudi 11 avril


Accueil > À la une > Distant formation and early evolution of the carbonaceous asteroid Ryugu : direct evidence from samples returned by Hayabusa2

Distant formation and early evolution of the carbonaceous asteroid Ryugu : direct evidence from samples returned by Hayabusa2

par Martrenchard-Barra Séverine - 22 septembre 2022 (modifié le 23 septembre 2022)

The Japanese Hayabusa2 mission (JAXA) has brought back samples from the carbonaceous primitive asteroid Ryugu. Thanks to the analyses of these samples by an international group led by Prof. Tomoki Nakamura (Tohoku Univ., Japan), it is possible to propose a scenario retracing the history of Ryugu, including its formation after the fragmentation of its parent asteroid.

The French laboratories involved are IAS, ICP, IJCLab, ISMO (Paris-Saclay University/CNRS), Synchrotron SOLEIL, IMPMC (Sorbonne-University/CNRS/MNHN), IPAG (Univ. Grenoble-Alpes/CNRS), IPGP (Univ. Paris Cité/CNRS) and LESIA (Paris-Meudon Observatory/CNRS), with the support of the CNES.

Ryugu samples contain minerals (hydrated silicates, carbonates, magnetite) as well as organic materials and water with CO2. A small proportion of Ryugu’s surface minerals formed near the Sun. Ryugu has a composition remarkably similar to the Orgueil meteorite, which fell in France in 1864 and is preserved at the MNHN in Paris. Orgueil belongs to a rare class of meteorites and it is used as a reference for the average composition of the Solar System. The samples from Ryugu thus offer a unique insight into this type of primitive materials.

The primordial magnetic field recorded in the magnetic minerals of Ryugu suggests that its parent asteroid formed in regions far from the Sun. A numerical simulation, based on the measured properties of the Ryugu samples, suggests that the parent body of Ryugu was 100 km in size and formed 2 million years after the formation of the Solar System. Over the 3 million years that followed, its temperature rose up to about 50°C, resulting in chemical reactions between water and rock. Subsequently, an impactor (at most 10 km in size) destroyed Ryugu’s parent body. Present-day Ryugu formed from material that was far from the impact point.

The full text of the JAXA press release :
https://global.jaxa.jp/press/2022/09/20220923-1_e.html.

The research results by the Hayabusa2 « Initial Analysis of Stones » Team (led by Prof. Tomoki Nakamura, Tohoku University) were published in Science on Thursday, September 22 :
T. Nakamura et al., Science 10.1126/science.abn8671 (2022).

JPEG - 63 kio
Optical micrograph of the largest sample C0002 analyzed
JPEG - 42.5 kio
Asteroid Ryugu photographed from a distance of about 20 km.

Dans la même rubrique :