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Asteroid split caused by dizzying spin rate
AMANDA DOYLE
ASTRONOMY NOW
Posted: 28 March 2012


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Asteroids that travel through the Solar System close to a companion but not as a bound binary pair could still have shared a common origin, perhaps even spinning apart from one single object, report astronomers at the National Astronomy Meeting in Manchester this week.

Asteroids spin as they travel along their orbits, and this rotation rate can be changed by the Yarkovsky–O'Keefe–Radzievskii–Paddack (YORP) effect. The YORP effect occurs when radiation emitted by small bodies also carries away momentum. If the YORP effect causes changes that go beyond the spin limit of the asteroid, then it can cause the asteroid to change shape. It can also result in a single asteroid being pulled apart to become a binary asteroid (read our earlier story Fast spinning asteroids spawn new generation here)


An artist’s impression of a double asteroid. Image: ESO

If one member of an asteroid binary is significantly smaller than the other, and this secondary comes close enough to the larger for gravitational interactions to occur, then it is possible for that the secondary asteroid will break free. The two asteroids then continue on their journey around the Sun in similar, but separate, orbits.

Simulations of the orbits of unbound asteroid pairs show that many of them would have had close encounters with each other less than a million years ago. However, this is still not sufficient evidence to prove that they originated from one asteroid.

In order to confirm a common origin, then the composition of the two asteroids needs to be measured, and this can be done using spectroscopy. Samuel Duddy from the University of Kent, along with his colleagues, made spectroscopic observations of several of these unbound asteroid pairs using the 4.2 metre William Herschel telescope and the 3.6 metre New Technology Telescope.

Duddy detailed the results of these observations at the National Astronomy Meeting this week where he revealed that the asteroid duo (7343) Ockeghem and (154634) 2003 XX38 have very similar compositions, which strongly suggests that they have a common origin. In addition, both asteroids are of the same taxonomic type.

While there were other convincing examples, not all of the binary pairs had matching compositions, which indicates that there must be more than one method of formation for asteroid pairs.

The Planets
From tiny Mercury to distant Neptune and Pluto, The Planets profiles each of the Solar System's members in depth, featuring the latest imagery from space missions. The tallest mountains, the deepest canyons, the strongest winds, raging atmospheric storms, terrain studded with craters and vast worlds of ice are just some of the sights you'll see on this 100-page tour of the planets.
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Hubble Reborn
Hubble Reborn takes the reader on a journey through the Universe with spectacular full-colour pictures of galaxies, nebulae, planets and stars as seen through Hubble's eyes, along the way telling the dramatic story of the space telescope, including interviews with key scientists and astronauts.
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3D Universe
Witness the most awesome sights of the Universe as they were meant to be seen in this 100-page extravaganza of planets, galaxies and star-scapes, all in 3D!
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