April 24, 2024

Samples From Asteroid Ryugu Shed New Light on Solar System History

Japans Hayabusa2 mission to asteroid Ryugu. Credit: JAXA
It has been nearly two years given that Japanese objective Hayabusa2 returned to Earth, samples from asteroid Ryugu are still exposing valuable details about the history of the early solar system. A new study reveals the isotopic composition of zinc and copper of asteroid Ryugu. According to the isotopic signatures, Ryugus composition is close to Ivuna-like carbonaceous chondrites, and Ryugu-like product from the external solar system represent ~ 5-6% of Earths mass.
These results, by scientists from the Paris Globe Institute of Physics (Institut de Physique du Globe de Paris), Université Paris Cité, and CNRS, as part of an international consortium, are released today (December 12, 2022) in the journal Nature Astronomy.
Meteorites discovered on Earth offer researchers with samples representing the first moments of the planetary system. A major action forward was made with the return to Earth in December 2020 of the Hayabusa2 mission, operated by the Japanese space agency JAXA. It restored 5 grams of fragments from the asteroid Ryugu, providing the possibility of analyzing samples unchanged by their arrival and remain on Earth.

Samples of asteroid Ryugu evaluated at IPGP Credit: © IPGP.
The very first analyses, performed by a global group, consisting of researchers from the Paris Globe Institute of Physics, Université Paris Cité, and the CNRS, have revealed that the structure of the asteroid Ryugu is close to that of Ivuna-like carbonaceous chondrites (CI)– the most chemically primitive meteorites, and thought about to have the composition closest to the Sun. However, some isotopic signatures (e.g., titanium and chromium) overlap with other groups of carbonaceous chondrites, so the information of the link between Ryugu and CI chondrites are not yet totally comprehended.
Zinc and copper are 2 reasonably unstable elements, and are crucial elements to study the procedures of accretion of volatiles during the formation of telluric worlds. The various groups of carbonaceous chondrites reveal distinct zinc and copper isotopic compositions, with the CI chondrites being the more enriched in unpredictable elements. By performing additional analyzes of the zinc and copper isotopic structure of Ryugu, the scientists had access to an important tool for studying the origin of the asteroid.
The worldwide team showed, in a study published on December 12th, 2022 in the journal Nature Astronomy and led by Marine Paquet and Frédéric Moynier, cosmochemists at the IPGP, that the isotopic ratios of copper and zinc in the samples from Ryugu were identical to CI chondrites but various from all other kinds of meteorites. By lastly validating the similarity between Ryugu and CI chondrites, this study develops that these primitive samples from Ryugu represent the very best quote of the solar composition to date for copper and zinc.
Finally, the zinc isotopic structure of Ryugu can likewise be utilized to study the accretional history of moderately volatile elements on Earth, which are vital for the development of planetary habitability. The research study likewise shows that the contribution of Ryugu-like product represents about 5% of the Earths mass.
Reference: “Contribution of Ryugu-like material to Earths unpredictable stock by Cu and Zn isotopic analysis” by Marine Paquet, Frederic Moynier, Tetsuya Yokoyama et al., 12 December 2022, Nature Astronomy.DOI: 10.1038/ s41550-022-01846-1.

A new research study reveals the isotopic structure of zinc and copper of asteroid Ryugu. According to the isotopic signatures, Ryugus composition is close to Ivuna-like carbonaceous chondrites, and Ryugu-like material from the external solar system accounts for ~ 5-6% of Earths mass.
By carrying out additional analyzes of the zinc and copper isotopic composition of Ryugu, the researchers had access to a vital tool for studying the origin of the asteroid.