The near-infrared spectrometer on board the Japanese Hayabusa spacecraft found a variation of more than 10% in albedo and absorption band depth in the surface reflectance of asteroid 25143 Itokawa. Spectral shape over the 1-micrometer absorption band indicates that the surface of this body has an olivine-rich mineral assemblage potentially similar to that of LL5 or LL6 chondrites. Diversity in the physical condition of Itokawa\u27s surface appears to be larger than for other S-type asteroids previously explored by spacecraft, such as 433 Eros
There has been a long-standing problem that the parent bodies of ordinary chondrites, the most abund...
The surface composition of S-type asteroids can be determined using band parameters extracted from t...
We obtained color images of near-Earth asteroid 25143 Itokawa by the Hayabusa multiband imaging came...
A photometric analysis of the S-type Asteroid 25143 Itokawa is performed over multiple wavelengths r...
In March 2001, the Hayabusa spacecraft target, Asteroid 25143 Itokawa, made its final close approach...
International audienceOn 27 June 2018, JAXA's Hayabusa2 spacecraft arrived at a distance of 20 km fr...
Olivine is one of the main abundant mineral in the Solar System, and the determination of its abunda...
International audienceWe report recent results of the surface composition of asteroid 162173 Ryugu f...
International audienceAsteroids, and more globally small bodies, are keys to unravel the origin and ...
We present results of a ground-based observational study of the Hayabusa mission target near-Earth A...
Asteroids that are targets of spacecraft missions are interesting because they present us with an op...
International audienceOn 27 June 2018, JAXA's Hayabusa2 spacecraft arrived at a distance of 20 km fr...
M-type asteroids, as defined in the Tholen taxonomy (Tholen, D.J. [1984]. Asteroid Taxonomy from Clu...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
There has been a long-standing problem that the parent bodies of ordinary chondrites, the most abund...
The surface composition of S-type asteroids can be determined using band parameters extracted from t...
We obtained color images of near-Earth asteroid 25143 Itokawa by the Hayabusa multiband imaging came...
A photometric analysis of the S-type Asteroid 25143 Itokawa is performed over multiple wavelengths r...
In March 2001, the Hayabusa spacecraft target, Asteroid 25143 Itokawa, made its final close approach...
International audienceOn 27 June 2018, JAXA's Hayabusa2 spacecraft arrived at a distance of 20 km fr...
Olivine is one of the main abundant mineral in the Solar System, and the determination of its abunda...
International audienceWe report recent results of the surface composition of asteroid 162173 Ryugu f...
International audienceAsteroids, and more globally small bodies, are keys to unravel the origin and ...
We present results of a ground-based observational study of the Hayabusa mission target near-Earth A...
Asteroids that are targets of spacecraft missions are interesting because they present us with an op...
International audienceOn 27 June 2018, JAXA's Hayabusa2 spacecraft arrived at a distance of 20 km fr...
M-type asteroids, as defined in the Tholen taxonomy (Tholen, D.J. [1984]. Asteroid Taxonomy from Clu...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
There has been a long-standing problem that the parent bodies of ordinary chondrites, the most abund...
The surface composition of S-type asteroids can be determined using band parameters extracted from t...
We obtained color images of near-Earth asteroid 25143 Itokawa by the Hayabusa multiband imaging came...