[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.