We use the observed effects of solar wind ion irradiation and the accumulation of solar flare particle tracks recorded in Itokawa grains to constrain the rates of space weathering and yield information about regolith dynamics. The track densities are consistent with exposure at mm depths for 104-105 years. The solar wind damaged rims form on a much faster timescale, <10(exp 3) years
Introduction: In a remarkable engineering achievement, the JAXA space agency successfully recovered ...
Context. The space weathering timescales of near-Earth S-type asteroids have been investigated using...
Analytical TEM observations of Itokawa grains reported to date show complex solar wind ion processin...
Space weathering processes such as solar wind irradiation and micrometeorite impacts are known to al...
Exposure to solar wind irradiation and micrometeorite impacts alter the properties of regolith mater...
The rates of space weathering processes are poorly constrained for asteroid surfaces, with recent es...
Mineral grains in lunar and asteroidal regolith samples provide a unique record of their interaction...
Space weathering effects on airless bodies result largely from micrometeorite impacts and solar wind...
Space weathering alters the chemistry, microstructure, and spectral proper-ties of grains on the sur...
Samples returned from the moon and Asteroid Itokawa by NASA's Apollo Missions and JAXA's Hayabusa Mi...
Limited samples are available for the study of space weathering effects on airless bodies. The grain...
Regolith grains returned by the Hayabusa mission to asteroid 25143 Itokawa provide the only samples ...
Mineral grains in lunar and asteroidal regolith samples provide a unique record of their interaction...
Context. The space weathering timescale of near-Earth S-type asteroids has been investigated by seve...
Regolith particles from airless bodies preserve a record of the space weathering processes that occu...
Introduction: In a remarkable engineering achievement, the JAXA space agency successfully recovered ...
Context. The space weathering timescales of near-Earth S-type asteroids have been investigated using...
Analytical TEM observations of Itokawa grains reported to date show complex solar wind ion processin...
Space weathering processes such as solar wind irradiation and micrometeorite impacts are known to al...
Exposure to solar wind irradiation and micrometeorite impacts alter the properties of regolith mater...
The rates of space weathering processes are poorly constrained for asteroid surfaces, with recent es...
Mineral grains in lunar and asteroidal regolith samples provide a unique record of their interaction...
Space weathering effects on airless bodies result largely from micrometeorite impacts and solar wind...
Space weathering alters the chemistry, microstructure, and spectral proper-ties of grains on the sur...
Samples returned from the moon and Asteroid Itokawa by NASA's Apollo Missions and JAXA's Hayabusa Mi...
Limited samples are available for the study of space weathering effects on airless bodies. The grain...
Regolith grains returned by the Hayabusa mission to asteroid 25143 Itokawa provide the only samples ...
Mineral grains in lunar and asteroidal regolith samples provide a unique record of their interaction...
Context. The space weathering timescale of near-Earth S-type asteroids has been investigated by seve...
Regolith particles from airless bodies preserve a record of the space weathering processes that occu...
Introduction: In a remarkable engineering achievement, the JAXA space agency successfully recovered ...
Context. The space weathering timescales of near-Earth S-type asteroids have been investigated using...
Analytical TEM observations of Itokawa grains reported to date show complex solar wind ion processin...