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Image of Itokawa from the Hayabusa spacecraft
Image of Itokawa from the Hayabusa spacecraft
Schematic of Itokawa's two lobes separated from each other. Their divergent densities suggest that these were stand-alone bodies that came into contac
Schematic of Itokawa's two lobes separated from each other. Their divergent densities suggest that these were stand-alone bodies that came into contact later on, making the rubble pile also a likely contact binary.
Preliminary shape model of Itokawa based on radar observations by Goldstone and Arecibo
Preliminary shape model of Itokawa based on radar observations by Goldstone and Arecibo
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Image: Asteroid 2006DP14
Image: Asteroid 2006DP14
Image: The VLT images the very faint Near Earth Object 2009 FD
Image: The VLT images the very faint Near Earth Object 2009 FD
Image: Comet Hartley 2
Image: Comet Hartley 2
Radar image of (388188) 2006 DP14 recorded by a DSN antenna
Radar image of (388188) 2006 DP14 recorded by a DSN antenna