On December 13 2012, a lunar probe called Chang'e-2 rendezvoused with asteroid 4179 Toutatis as the rock, bigger than a city block, swept by Earth at a distance of around seven million kilometres.
Describing the encounter in detail in the journal Scientific Reports, Chinese scientists said the flyby was brief but highly successful, the result of seven months of preparation after Chang'e-2 had completed its primary mission of orbiting the Moon.
Advancing at more than 38,000 kilometres per hour, the probe came within 770 metres of the asteroid's surface, returning pictures with a resolution better than three metres per pixel.
The astronomers also saw boulders and small gravel-like stones called regolith sliding over its surface, which suggest that Toutatis is not so much a single, solid rock but more an assembly of rubble.
"The rubble-pile structure is essentially a normal situation for most of the smaller asteroids" under a kilometre across, said Ji Jianghui of the Chinese Academy of Sciences in Beijing.
"This is also the case for Toutatis. In this structure, the asteroids are not a single rock but a loose collection of fragments under the influence of gravity, which means that it is an agglomeration of gravitationally-bound chunks," Ji said in an email exchange with AFP.
Toutatis is one of the biggest "potentially hazardous asteroids," or PHAs, or rogue rocks whose orbit can bring them close to our planet.
As a result, it has been closely followed by telescopes and radar on Earth.
It came by Earth in 1992, 1996, 2000, 2004, 2008 and 2012, but will not approach so close until 2069.
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