Add to ORKGThe petrographic study of Itokawa particle, RA-QD02-0127 has been performed by SEM-EDS and optical microscope observations. The purpose of this study is to understand better the metamorphic and impact shock history of asteroid Itokawa, and other S-class asteroids
Y-82094 is an ungrouped type 3.2 carbonaceous chondrite, with abundant chondrules making 78 vol.% of...
Limited samples are available for the study of space weathering effects on airless bodies. The grain...
In situ extrate rrestrial samples returned for study (e.g., from the Moon) are crucial in understand...
We studied seven Itokawa particles provided by the Japan Aerospace Exploration Agency (JAXA) as firs...
JAXA Hayabusa mission success-fully returned particles of the asteroid Itokawa to the earth in 2010....
We have been analyzing Itokawa samples in order to definitively establish the degree of shock experi...
Introduction: In a remarkable engineering achievement, the JAXA space agency successfully recovered ...
The lattice distortion of minerals included in a thin section of meteorites was measured by a newly ...
A strong link between Itokawa particles and LL chondrites was confirmed by preliminary examinations ...
We have been analyzing Itokawa samples in order to definitively establish the degree of shock experi...
We requested and have been approved for 5 Hayabusa samples in order definitively establish the degre...
The analysis of ateroid’s surface grains allows to match remote observations and modeling of its his...
In 2010, fine regolith particles on asteroid Itokawa were recovered by the Hayabusa mission. The thr...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
One of the fundamental aspects of any astromaterial is its shock history, since this factor elucidat...
Y-82094 is an ungrouped type 3.2 carbonaceous chondrite, with abundant chondrules making 78 vol.% of...
Limited samples are available for the study of space weathering effects on airless bodies. The grain...
In situ extrate rrestrial samples returned for study (e.g., from the Moon) are crucial in understand...
We studied seven Itokawa particles provided by the Japan Aerospace Exploration Agency (JAXA) as firs...
JAXA Hayabusa mission success-fully returned particles of the asteroid Itokawa to the earth in 2010....
We have been analyzing Itokawa samples in order to definitively establish the degree of shock experi...
Introduction: In a remarkable engineering achievement, the JAXA space agency successfully recovered ...
The lattice distortion of minerals included in a thin section of meteorites was measured by a newly ...
A strong link between Itokawa particles and LL chondrites was confirmed by preliminary examinations ...
We have been analyzing Itokawa samples in order to definitively establish the degree of shock experi...
We requested and have been approved for 5 Hayabusa samples in order definitively establish the degre...
The analysis of ateroid’s surface grains allows to match remote observations and modeling of its his...
In 2010, fine regolith particles on asteroid Itokawa were recovered by the Hayabusa mission. The thr...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
One of the fundamental aspects of any astromaterial is its shock history, since this factor elucidat...
Y-82094 is an ungrouped type 3.2 carbonaceous chondrite, with abundant chondrules making 78 vol.% of...
Limited samples are available for the study of space weathering effects on airless bodies. The grain...
In situ extrate rrestrial samples returned for study (e.g., from the Moon) are crucial in understand...