On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective

Presented here are the observations and interpretations from a comprehensive analysis of 16 representative particles returned from the C-type asteroid Ryugu by the Hayabusa2 mission. On average Ryugu particles consist of 50% phyllosilicate matrix, 41% porosity and 9% minor phases, including organic matter. The abundances of 70 elements from the particles are in close agreement with those of CI chondrites. Bulk Ryugu particles show higher δ18O, Δ17O, and ε54Cr values than CI chondrites. As such, Ryugu sampled the most primitive and least-thermally processed protosolar nebula reservoirs. Such a finding is consistent with multi-scale H-C-N isotopic compositions that are compatible with an origin for Ryugu organic matter within both the protosolar nebula and the interstellar medium. The analytical data obtained here, suggests that complex soluble organic matter formed during aqueous alteration on the Ryugu progenitor planetesimal (several 10’s of km), <2.6 Myr after CAI formation. Subsequently, the Ryugu progenitor planetesimal was fragmented and evolved into the current asteroid Ryugu through sublimation

A pristine record of outer Solar System materials from asteroid Ryugu’s returned sample

Volatile and organic-rich C-type asteroids may have been one of the main sources of Earth’s water. Our best insight into their chemistry is currently provided by carbonaceous chondritic meteorites, but the meteorite record is biased: only the strongest types survive atmospheric entry and are then modified by interaction with the terrestrial environment. Here we present the results of a detailed bulk and microanalytical study of pristine Ryugu particles, brought to Earth by the Hayabusa2 spacecraft. Ryugu particles display a close compositional match with the chemically unfractionated, but aqueously altered, CI (Ivuna-type) chondrites, which are widely used as a proxy for the bulk Solar System composition. The sample shows an intricate spatial relationship between aliphatic-rich organics and phyllosilicates and indicates maximum temperatures of ~30 °C during aqueous alteration. We find that heavy hydrogen and nitrogen abundances are consistent with an outer Solar System origin. Ryugu particles are the most uncontaminated and unfractionated extraterrestrial materials studied so far, and provide the best available match to the bulk Solar System composition

A dehydrated space-weathered skin cloaking the hydrated interior of Ryugu

Without a protective atmosphere, space-exposed surfaces of airless Solar System bodies gradually experience an alteration in composition, structure and optical properties through a collective process called space weathering. The return of samples from near-Earth asteroid (162173) Ryugu by Hayabusa2 provides the first opportunity for laboratory study of space-weathering signatures on the most abundant type of inner solar system body: a C-type asteroid, composed of materials largely unchanged since the formation of the Solar System. Weathered Ryugu grains show areas of surface amorphization and partial melting of phyllosilicates, in which reduction from Fe3+ to Fe2+ and dehydration developed. Space weathering probably contributed to dehydration by dehydroxylation of Ryugu surface phyllosilicates that had already lost interlayer water molecules and to weakening of the 2.7 µm hydroxyl (–OH) band in reflectance spectra. For C-type asteroids in general, this indicates that a weak 2.7 µm band can signify space-weathering-induced surface dehydration, rather than bulk volatile loss

A case of drug-induced interstitial pneumonia caused by repeated exposure to bepridil

The patient was a 78-year-old man. In August 2007, he underwent catheter ablation for atrial fibrillation after taking bepridil for 3 weeks. Soon after the ablation, he experienced frequent atrial extrasystoles and began taking bepridil again on the day he left the hospital. Six days after discharge, he was readmitted to our hospital with dyspnea and was diagnosed with acute heart failure. The patient had no recurrence of atrial fibrillation, so the administration of bepridil was stopped. His dyspnea was eased using standard therapy for heart failure and he was discharged from our hospital. In March 2011, he had a recurrence of atrial fibrillation and was readmitted to our hospital. The administration of bepridil was initiated to defibrillate the atrial fibrillation. Although bepridil stopped the atrial fibrillation by the third day, he presented with dyspnea and fever on the fourth day. A chest radiograph showed bilateral interstitial patterns that radiated from the pulmonary hilum. He was treated for acute heart failure and bacterial pneumonia, but this was ineffective. We suspected that the interstitial pneumonia was caused by bepridil. Corticosteroid therapy dramatically improved his symptoms. This was a rare case of acute drug-induced interstitial pneumonia caused by repeated exposure to bepridil

-4 Heart Asia Roles of ghrelin in left-ventricular remodelling after acute myocardial infarction

. Multivariate regression analysis showed that ghrelin on day 14 is a significant predictor of LV remodelling after AMI (b¼ +0.44, p¼0.001). Conclusion To our knowledge, this is the first report that shows a relation between circulating ghrelin after AMI and the progression of LV remodelling in the chronic phase. The elevation of ghrelin after AMI might be a compensatory mechanism to attenuate LV remodelling

First asteroid gas sample delivered by the Hayabusa2 mission: A treasure box from Ryugu

The Hayabusa2 spacecraft returned to Earth from the asteroid 162173 Ryugu on 6 December 2020. One day after the recovery, the gas species retained in the sample container were extracted and measured on-site and stored in gas collection bottles. The container gas consists of helium and neon with an extraterrestrial 3He/4He and 20Ne/22Ne ratios, along with some contaminant terrestrial atmospheric gases. A mixture of solar and Earth's atmospheric gas is the best explanation for the container gas composition. Fragmentation of Ryugu grains within the sample container is discussed on the basis of the estimated amount of indigenous He and the size distribution of the recovered Ryugu grains. This is the first successful return of gas species from a near-Earth asteroid.ISSN:2375-254