Itokawa / Science

Science · Itokawa

What the research says about Itokawa

These are six research papers, all free to read on arXiv, about Itokawa. 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.

Rotation period
12.1324hours2± 0.0001 h, from ground-based light curves 2001–2004.
Space-weathering timescale
≈ 1,000years4For boulder surfaces; range about 100 to 10,000 years.
01

Size, shape & spin

2 papers

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

[1]2005astro-phPreprint

Thermal infrared observations of the Hayabusa spacecraft target asteroid 25143 Itokawa

T. G. Mueller, T. Sekiguchi & M. Kaasalainen

What they foundItokawa's effective diameter is about 0.32 km with an albedo of about 0.19, and its high thermal inertia points to a bare-rock surface.

Why it mattersMeasured before Hayabusa arrived, it later helped interpret the mission's close-up views.
What they studied

Thermal-infrared observations from the ESO 3.6 m telescope in July 2004.

arXiv:astro-ph/0509434Abstract (opens arXiv)PDF (opens arXiv)
[2]2018astro-ph.EPPreprint

Ground-based lightcurve observation campaign of (25143) Itokawa between 2001 and 2004

Setsuko Nishihara, Kouhei Kitazato, Masanao Abe & 9 others

What they foundItokawa spins once every 12.1324 hours.

Why it mattersPrecise rotation data supported Hayabusa's navigation and later studies of spin changes.
What they studied

Ground-based light curves from three telescopes, 2001 to 2004.

Source for: Rotation period

02

Surface & composition

3 papers

What Itokawa is made of and how its surface behaves.

[3]2019astro-ph.EPPeer-reviewed

The Global Surface Roughness of 25143 Itokawa

Hannah C. M. Susorney, Catherine L. Johnson, Olivier S. Barnouin & 4 others

What they foundFirst global roughness maps of Itokawa show fine material sliding downhill into low areas and big blocks left on highs, unlike Eros, where craters dominate.

Why it mattersIt shows tiny asteroids are reshaped by movement of surface material, not just impacts.
What they studied

Analysis of Hayabusa shape data at 8 to 32 m scales.

[4]2022astro-ph.EPPeer-reviewed

Estimation of space weathering timescale on (25143) Itokawa: Implications on its rejuvenation process

Sunho Jin & Masateru Ishiguro

What they foundSpace weathering darkens Itokawa's boulders in about 1,000 years (range 100 to 10,000).

Why it mattersSuch a short timescale means fresh-looking areas must have been disturbed very recently.
What they studied

Counting bright impact marks on boulders in Hayabusa AMICA images.

Source for: Space-weathering timescale

[5]2025astro-ph.EPPeer-reviewed

Simulation of Impact-induced seismic shaking on asteroid (25143) Itokawa to address its resurfacing process

Sunho Jin & Masateru Ishiguro

What they foundShaking from the impact that formed the 8-m Kamoi crater could have been strong enough to move surface material and refresh parts of Itokawa.

Why it mattersIt offers an explanation for the mix of fresh and old terrain.
What they studied

3D seismic-wave and landslide simulations.

03

Orbit & dynamics

1 paper

How Itokawa moves, and the gravity and sunlight forces that shape its path.

[6]2008astro-phPreprint

Effect of Density Inhomogeneity on YORP: The case of Itokawa

D. J. Scheeres

What they foundA centre-of-mass shift of about 10 m could flip the predicted sign of the YORP spin change on Itokawa, and the theory favours a shift toward the neck.

Why it mattersIt suggests Itokawa's interior isn't uniform.
What they studied

Theory applied to the Itokawa shape model.

New research

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

RSS feed

No new papers on Itokawa this week. We check arXiv every week.

How we choose papers

We search arXiv for Itokawa 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.