How are Asteroids Like Geckos?

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Asteroids are strange celestial objects, particularly the smaller spinning variety, like the little potato-shaped asteroid named Itokawa. Scientists have been puzzling over what holds these smaller asteroids together, since they are too small for gravity to overcome the centripetal forces and hold the various bits of rubble as one to make an asteroid. And it turns out that Itokawa and its siblings have something in common with the gecko.

The puzzle is based on 2005 data collected by Japan’s Hayabusa mission, which showed that at the rate at which Itokawa is spinning, the centripetal forces should overcome gravity and the pieces should fly off into space. But instead, they remain intact, giving Itokawa its unique spud-like shape. What is making the difference? Suggestions have included pressure arising from radiation from the sun, and friction and electrostatic forces occurring in the ionized dust.

BIG PIC GALLERY: Japan’s Hayabusa mission made it into the Discovery News’ Best Space Probe Photographers of the Decade gallery.

Now a new analysis by a team of University of Colorado scientists suggests that the real culprit might be van der Waals forces. Named after Dutch scientist Johannes van der Waals, this is the force that causes attraction or repulsion between molecules in chemistry, that cannot be attributed to the usual chemical bonds or electrostatic interactions of ions. It’s not a force that gets bandied about much these days in astrophysics, but here on Earth, it’s the force behind geckos’ ability to “adhere” to smooth surfaces even at bizarre angles. Apparently it’s the creature’s body orientation, and resulting change in gravity acting upon it, that triggers the gecko grip.

WATCH VIDEO: The angle of a surface – not its slipperiness – triggers when geckos turn on their superhero-like ability to walk on walls and ceilings.

Those same van der Waals forces kick in in the latter stages of small asteroid evolution, according to the Colorado scientists, after the spinning objects have thrown off larger rocks that would incur larger gravitational effects. Eventually all that is left is the smaller bits of rubble, which act much like molecules and form bonds via van der Waals.

It’s an intriguing notion, and Daniel Scheeres, who heads the Colorado team, thinks it might also be able to shed some light on how Saturn’s rings may have formed — those rings, after all, are made up almost entirely of dust and tiny bits of rubble that also seem to be strangely attracted to one another. So the humble gecko could hold the secret not just to a possible dry glue here on Earth, but to how certain celestial objects form as well.

Publication: Scaling forces to asteroid surfaces: The role of cohesion, Scheeres et al., 2010, arXiv:1002.2478v1 [astro-ph.EP] via arXiv blog.

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