Itokawa is the first asteroid from which samples were brought to Earth for analysis. This feat was achieved by Japanese space probe Hayabusa which touched down on the asteroid in November 2005 and returned to Earth in June 2010.
Hayabusa’s close-up observations of the asteroid and the subsequent analysis of its dust in labs on Earth support the conclusion that Itokawa is part of what remains from a much larger object that was shattered by a collision. The dust also confirms that S-type (this refers to the asteroid’s color spectrum) asteroids like Itokawa, which are the most common type of asteroid in the inner main belt, are the source of the most common kind of meteorite found on Earth: the ordinary chondrite.
Scientists think Itokawa is not solid, but rather is a rubble pile, an agglomeration of rocks loosely held together by their mutual gravity. Few craters are visible, presumably because any impact energetic enough to create a crater shakes rocks loose and they fill the hole.
One sign that the asteroid was once part of a much larger object is that many of the captured dust particles show signs of having slowly cooled after forming deep inside a rocky object at a temperature of some 1,500 degrees Fahrenheit (800 degrees Celsius). For this to have occurred, the diameter of the rocky object would have to have been greater than 20 km (12 miles), whereas Itokawa’s longest dimension is only 0.5 km (0.3 miles).
Another clue is that the largest boulder found on Itokawa is about 50 m (160 feet) across, which is believed to be too big to have been ejected by the impact that created the asteroid’s largest crater. Scientists think the rock is a fragment of whatever cataclysmic event resulted in Itokawa’s current construction.
Writing in the journal Science, Hayabusa’s science team described the asteroid’s shape as resembling a sea otter, with one distinct part designated as the head and the other, larger part designated as the body. One of the scenarios that the team cited as most likely to explain this is that after Itokawa’s parent body was shattered, the slight mutual gravity of the fragments brought them together into two or more rubble piles, and two of these piles eventually bumped gently into each other and stuck together. Another possibility is that Itokawa was originally one rubble pile, and a large impact temporarily broke off a chunk of it until gravity brought it back and the two parts became reattached.
Itokawa’s orbit around the sun crosses those of both Earth and Mars.
Credit : NASA Science
Picture Credit : Google
