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20142026
most citedPresolar stardust in asteroid Ryugu

36 citations · 154 across the 17 of their papers we have counts for

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Showing astro-ph.EPShow all

16 papers · 1 filter

astro-ph.EP2026★ 1 cited

Characteristics of natural remanence records in fine-grained particles returned from asteroid Ryugu

Masahiko Sato, Yuki Kimura, Tadahiro Hatakeyama +25

Particles collected from the asteroid Ryugu by the Hayabusa2 spacecraft offer a unique opportunity to investigate the magnetic record of the primitive solar system, as any terrestr…

astro-ph.EP2024★ 34 cited

The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites

Fridolin Spitzer, Thorsten Kleine, Christoph Burkhardt +88

The isotopic compositions of samples returned from Cb-type asteroid Ryugu and Ivuna-type (CI) chondrites are distinct from other carbonaceous chondrites, which has led to the sugge…

astro-ph.EP2024

Spectro-photometry of Phobos simulants: II. Effects of porosity

Antonin Wargnier, Olivier Poch, Giovanni Poggiali +13

Surface porosity has been found to be an important property for small bodies. Some asteroids and comets can exhibit an extremely high surface porosity in the first millimeter layer…

astro-ph.EP2024

Study of hydrated asteroids via their polarimetric properties at low phase angles

Jooyeon Geem, Masateru Ishiguro, Hiroyuki Naito +11

Context. Ch-type asteroids are distinctive among other dark asteroids in that they exhibit deep negative polarization branches (NPBs). Nevertheless, the physical and compositional…

astro-ph.EP2024

Spectro-photometry of Phobos simulants: I. Detectability of hydrated minerals and organic bands

Antonin Wargnier, Thomas Gautier, Alain Doressoundiram +12

Previous observations of Phobos and Deimos, the moons of Mars, have improved our understanding of these small bodies. However, their formation and composition remain poorly constra…

astro-ph.EP2024★ 1 cited

Microscale Hydrogen, Carbon, and Nitrogen Isotopic Diversity of Organic Matter in Asteroid Ryugu

Larry R Nittler, Jens Barosch, Katherine Burgess +57

We report the H, C, and N isotopic compositions of microscale (0.2 to 2m) organic matter in samples of asteroid Ryugu and the Orgueil CI carbonaceous chondrite. Three regolith p…

astro-ph.EP2023★ 4 cited

Reproduction Experiments of Radial Pyroxene Chondrules Using a Gas-jet Levitation System under Reduced Conditions

Kana Watanabe, Tomoki Nakamura, Tomoyo Morita

Reproduction experiments of radial pyroxene (RP) chondrules were carried out using an Ar- or Ar gas-jet levitation system in a reducing atmosphere in order to simulat…

astro-ph.EP2022★ 36 cited

Presolar stardust in asteroid Ryugu

Jens Barosch, Larry R. Nittler, Jianhua Wang +121

We have conducted a NanoSIMS-based search for presolar material in samples recently returned from C-type asteroid Ryugu as part of JAXA's Hayabusa2 mission. We report the detection…

astro-ph.EP2021★ 9 cited

High-Resolution Observations of Bright Boulders on Asteroid Ryugu: 1. Size Frequency Distribution and Morphology

Chiho Sugimoto, Eri Tatsumi, Yuichiro Cho +34

The near-Earth asteroid (162173) Ryugu displays a Cb-type average spectrum and a very low average normal albedo of 0.04. Although the majority of boulders on Ryugu have reflectance…

astro-ph.EP2021★ 12 cited

High-Resolution Observations of Bright Boulders on Asteroid Ryugu: 2. Spectral Properties

Chiho Sugimoto, Eri Tatsumi, Yuichiro Cho +34

Many small boulders with reflectance values higher than 1.5 times the average reflectance have been found on the near-Earth asteroid 162173 Ryugu. Based on their visible wavelength…

astro-ph.EP2019★ 4 cited

ASIME 2018 White Paper. In-Space Utilisation of Asteroids: Asteroid Composition -- Answers to Questions from the Asteroid Miners

Amara L. Graps, Angel Abbud-Madrid, Paul Abell +41

In keeping with the Luxembourg government's initiative to support the future use of space resources, ASIME 2018 was held in Belval, Luxembourg on April 16-17, 2018. The goal of ASI…

astro-ph.EP2018★ 8 cited

Nebular history of an ultrarefractory phase bearing CAI from a reduced type CV chondrite

Takashi Yoshizaki, Daisuke Nakashima, Tomoki Nakamura +4

Ultrarefractory (UR) phases in CAIs could have formed at higher T compared to common CAI minerals and thus they potentially provide constraints on very high-T processes in the sola…

astro-ph.EP2017★ 22 cited

On the impact origin of Phobos and Deimos III: resulting composition from different impactors

Francesco C. Pignatale, Sébastien Charnoz, Pascal Rosenblatt +3

The origin of Phobos and Deimos in a giant impact generated disk is gaining larger attention. Although this scenario has been the subject of many studies, an evaluation of the chem…

astro-ph.EP2017★ 4 cited

Rotationally time-resolved vis-spectroscopy of (3200) Phaethon

Daisuke Kinoshita, Katsuhito Ohtsuka, Takashi Ito +4

Apollo-type NEA (3200) Phaethon, classified at the B/F-type taxonomy, probably the main mass of the Phaethon-Geminid stream complex (PGC), can be the most metamorphic C-complex ast…

astro-ph.EP2016★ 12 cited

The Formation and Evolution of Ordinary Chondrite Parent Bodies

Pierre Vernazza, Brigitte Zanda, Tomoki Nakamura +2

Ordinary chondrites (OCs) are by far the most abundant meteorites (80% of all falls). Their origin has long been the matter of a heated debate. About thirty years ago (e.g., Pellas…

astro-ph.EP2014★ 6 cited

Fast Rotation of a Sub-km-sized Near-Earth Object 2011 XA3

S. Urakawa, K. Ohtsuka, S. Abe +2

We present lightcurve observations and their multiband photometry for near-Earth object (NEO) 2011 XA3. The lightcurve has shown a periodicity of 0.0304 +- 0.0003 day (= 43.8 +- 0.…