Ryugu Samples Illuminate Terrestrial Weathering Effects On Primitive Meteorites
A groundbreaking study conducted by a team of international scientists has unveiled unprecedented insights into the nature of the asteroid Ryugu and shed light on the composition of water- and carbon-rich small bodies in the solar system.
Asteroids like Ryugu are remnants of planetary embryos that never reached larger sizes, making them invaluable windows into materials that formed in the early solar system. The study centered on laboratory measurements of the samples brought back to the Earth by the Hayabusa2 spacecraft in 2020. Led by the Japan Aerospace Exploration Agency (JAXA), Hayabusa2 aimed to uncover the true nature of Ryugu and explore how astrologists can use knowledge from meteorites to interpret telescopic observations of other hydrous asteroids.
Unlike meteorites derived from similar hydrous asteroids, the Ryugu samples avoided terrestrial alteration – the interaction with oxygen and water in the Earth’s atmosphere.
Reflectance spectroscopy, a primary technique linking laboratory analyses of meteorites to asteroid observations, was employed to compare fresh Ryugu samples with meteorites altered in terrestrial environments. The team successfully developed analytical procedures that avoided exposing the samples to Earth’s atmosphere, ensuring the preservation of their original conditions.
Previous studies suggested that Ryugu’s sample mineralogy resembled CI chondrites, the most primitive meteorites chemically. However, other studies have contradicted this by revealing a significant difference in reflectance spectra between Ryugu samples and CI chondrites. Further investigations in the new study indicated that heating CI samples under reducing conditions at 300 °C reproduced Ryugu’s sample mineralogy well, resulting in spectra closely matching those of Ryugu samples.
The findings challenge previous assumptions about the parent bodies of CI chondrites and underscore the susceptibility of primitive meteorite spectra to terrestrial weathering. The study suggests that actual CI chondrite parent bodies likely exhibit darker and flatter reflectance spectra than previously thought.
“This study opens new avenues for understanding the composition and evolution of small bodies in our solar system. By considering the impact of terrestrial weathering on meteorites, we can refine our interpretations of asteroid compositions and advance our knowledge of the solar system’s early history,” said Kana Amano, a former PhD student at the early Solar System evolution Research Group at Tohoku University and co-author of the paper.
Vis-NIR reflectance spectra of Ryugu and chondrite samples. (A and B) Ryugu coarse aggregate samples (TD1, TD2, and glossy coarse) and carbonaceous chondrite chip samples (Orgueil CI, Ivuna CI, Tagish Lake C2–ungrouped, Tarda C2–ungrouped, Murchison CM, Allende CV, Moss CO, and LAP 04721 CR2). Spectral data of Allende and Moss chondrites are cited from (40). The vertical gray lines indicate 0.48, 0.55, 0.70, and 0.86 μm in wavelength (b-, v-, w-, and x-bands, respectively) (6). Ryugu’s Vis-NIR reflectance spectra are darker than hydrated carbonaceous chondrites (A) and anhydrous carbonaceous chondrites (B). (C and D) Vis-NIR reflectance spectra of Ryugu powder aggregate samples and experimentally heated Orgueil (CI) powder samples. Ryugu’s dark and flat spectra are similar to those of Orgueil powder samples heated at 300° to 600°C. — Science
Details of Amano and her colleagues’ findings were published in the journal Science Advances on December 6, 2023.
Reassigning CI chondrite parent bodies based on reflectance spectroscopy of samples from carbonaceous asteroid Ryugu and meteorites, Science (open access)
Astrobiology, Astrochemistry,
