Itokawa (minor planet 25143)
 |
Image of Itokawa taken by Hayabusa
from a range of about 20 km |
A small asteroid that was the target of
the Japanese Hayabusa (MUSES-C) probe –
the first spacecraft to return a sample of material from an asteroid. 25143
Itokawa, also known as 1998 SF36, was discovered by LINEAR
in 1998 and is named after the late Hideo Itokawa, considered one of the
fathers of Japan's space program. It is both an Apollo
asteroid and a Mars-crosser and
appears to have an S-class composition.
The first images of Itokawa returned by Hayabusa proved surprising. The
asteroid's shape – similar to a knobbly potato – is not what
researchers had predicted based on radar images. Another asteroid mission,
NASA's NEAR-Shoemaker, visited the asteroid
Eros in 2000 and found it to be fairly
homogenous. This does not appear to be the case for Itokawa. Early pictures
of the asteroid appear to show hilly and rocky regions in addition to some
very smooth features. Itokawa's edges appear rounded, possibly the result
of eons of being pelted by other space objects. There also appears to be
some dust and rocks left over from impacts on the asteroid's surface. This
is another surprise because small asteroids, with such a small gravitational
pull, were not expected to havemuch in the way of regolith.
It is strongly suspected from its appearance that Itokawa may be a rubble-pile
asteroid.
| dimensions |
0.687 × 0.287 × 0.264 km |
| mass |
~4.8 × 1010 kg |
| spectral class |
S |
| rotational period |
12.5 hours |
| albedo |
0.53 |
| semimajor axis |
1.324 AU |
| perihelion |
0.953 AU |
| aphelion |
1.695 AU |
| eccentricity |
0.280 |
| inclination |
1.62° |
| orbital period |
556.36 days |
Related category
NOTABLE
ASTEROIDS, CENTAURS, AND KUIPER BELT OBJECTS
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