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Science · Ryugu

What the research says about Ryugu

These are six research papers, all free to read on arXiv, about Ryugu. We summarize each one in plain English from its abstract.

  • Papers 6
  • Topics 3
  • Reviewed Oct 24, 2026
  • Source arXiv.org
Illustrative · not to scale

Our own artist's impression. No figures are taken from the papers.

Known so far

Every number links to the paper it comes from.

Macroporosity
14%1± 4%, from the sizes of its boulders.
Craters over 20 m
77craters3Global catalogue from Hayabusa2 images.
01

Size, shape & spin

2 papers

How big Ryugu is, what shape it has and how it spins.

[1]2021astro-ph.EPPreprint

The Macroporosity of Rubble Pile Asteroid Ryugu and Implications for the Origin of Chondrules

William Herbst, James P. Greenwood & Teng Ee Yap

What they foundRyugu's boulders imply a macroporosity of about 14%, so its rocks average only about 1.38 g/cm³.

Why it mattersSuch light rock suggests dense, well-cemented pieces are rare inside Ryugu.
What they studied

Packing theory applied to Ryugu's measured boulder sizes.

Source for: Macroporosity

[2]2019astro-ph.EPPreprint

The Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process

Masatoshi Hirabayashi, Eri Tatsumi, Hideaki Miyamoto & 26 others

What they foundRyugu's smooth western bulge could have formed when it spun faster than about 3.75 hours per turn and part of it deformed.

Why it mattersIt suggests Ryugu once spun much faster than today.
What they studied

Finite-element modelling on the mission's shape model.

02

Surface & composition

1 paper

What Ryugu is made of and how its surface behaves.

[3]2022astro-ph.EPPeer-reviewed

The spatial distribution of impact craters on Ryugu

Naoyuki Hirata, Tomokatsu Morota, Yuichiro Cho & 40 others

What they foundA catalogue of 77 craters over 20 m across shows more craters at low latitudes and fewer in the western bulge.

Why it mattersThe uneven pattern implies a complicated geologic history.
What they studied

Hayabusa2 ONC images up to February 2019.

Source for: Craters over 20 m

03

Origins & history

3 papers

Where Ryugu came from and how it formed and changed over time.

[4]2022astro-ph.EPPeer-reviewed

Presolar stardust in asteroid Ryugu

Jens Barosch, Larry R. Nittler, Jianhua Wang & 121 others

What they foundRyugu samples contain presolar stardust: silicate, oxide, silicon carbide and carbon grains older than the Sun.

Why it mattersRyugu's material links it to the most primitive carbon-rich meteorites.
What they studied

NanoSIMS isotope mapping of samples returned by Hayabusa2.

[5]2024astro-ph.EPPeer-reviewed

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

Fridolin Spitzer, Thorsten Kleine, Christoph Burkhardt & 88 others

What they foundRyugu and CI-type meteorites share the same nickel isotope signature, distinct from other carbon-rich meteorites.

Why it mattersIt points to a shared birthplace or formation time for Ryugu's parent body and CI meteorites.
What they studied

Nickel isotope measurements of returned samples.

[6]2025astro-ph.EPPreprint

The molecular chemistry of nanoscale organic matter in asteroid Ryugu

Christian Vollmer, Demie Kepaptsoglou, Johannes Lier & 2 others

What they foundSome organic matter in Ryugu contains nitrogen-bearing groups and formed in the cold outer solar nebula.

Why it mattersCarbon-rich asteroids may have delivered life-relevant molecules to the early Earth.
What they studied

Electron-microscope spectroscopy of pristine samples at the nanoscale.

New research

New papers on Ryugu, checked weekly, summarized after a person reads it.

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How we choose papers

We search arXiv for Ryugu papers and keep the ones that add something new, are clearly written up and are relevant to a general reader. A person reads every abstract.

Our own words, our own drawings

Summaries are written by us from each paper’s abstract, not copied. Diagrams are our own simplified drawings, not figures from the papers.

Preprint vs. peer-reviewed

“Peer-reviewed” means arXiv lists a journal reference for the paper. Everything else is marked “Preprint”: shared openly, possibly before or without journal review.

Paper metadata courtesy of arXiv. Summaries written by us; read the original papers via the links. Paper metadata from arXiv.org, which does not endorse this site.