[meteorite-list] Fresh Spin on Solar Powered Asteroids
From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Apr 22 10:29:53 2004 Message-ID: <200309101945.MAA25987_at_zagami.jpl.nasa.gov> http://space.com/scienceastronomy/asteroid_spin_030910.html Fresh Spin on Solar Powered Asteroids By Robert Roy Britt space.com 10 September 2003 Collisions can send asteroids whirling and twirling. But what can really put space rocks into a spin is the subtle yet constant effect of sunlight. Strange as it might seem, solar heat can have a greater impact on whether and how a small asteroid rotates upon its own axis than do the explosive impacts that cleave them into existence in the first place. A new study on the effect seems to solve a mystery that began last fall. In September, MIT researcher Stephen Slivan announced odd orientations of 10 small asteroids in the Koronis family. All the rocks are chips off two larger blocks that collided at least two billion years ago. They range in size from 12 to 26 miles (20-40 kilometers). Slivan had expected each asteroid's spin axis to be randomly oriented, a result of the group's chaotic origin and myriad random smaller crashes that should have occurred since. Instead he found six of the rocks pointing one distinct direction and four in another. Reaction over time Another group of researchers looked into how this could have happened. They began with the knowledge that sunlight causes uneven heating on a space rock -- just as Earth's day side is warmed while the night side is cooler. The day side, especially the afternoon portion, re-radiates significantly more solar energy back into space, creating a recoil force. An asteroid's orbit around the Sun shifts over time due to this process, which can slow the rock down and cause it to drift off course. It's called the Yarkovsky effect, after the Russian engineer who came up with it around 1900. Some scientists have suggested the Yarkovsky effect could be employed to save Earth from a deadly impact. An incoming asteroid's path could be altered by simply painting the rock white and letting the Sun do the heavy lifting, providing there is a lengthy warning period. The Yarkovsky effect is most pronounced on smaller objects. Other research has shown that uneven heating shuttle's meteoroids -- baseball and boulder-sized bits created in asteroid crashes -- into certain solar system zones that serve as portals, guaranteeing the objects a shot at hitting Earth. YORP effect A similar presumed effect, named YORP (for Yarkovsky and some colleagues), long ago suggested that an asteroid's spin rate and orientation would also be altered by sunlight. But scientists always assumed the effect would be minor and, importantly, random. In the new research, the effect of sunlight on asteroids was simulated by in new computer model. The recoil effect, it turns out, can over the eons substantially alter an asteroid's rotation rate and axis orientation in semi-predictable ways, rather than just randomly. "Like the story about the tortoise and the hare, slow and steady sunlight wins the race over the fast-acting, but less effective, jolt of collisions between asteroids," said William Bottke, a study team member from the Southwest Research Institute. The effect can cause asteroids to be captured into special situations in which the wobble of the spin axis beats at the same frequency as the wobble of the rock's orbit around the Sun, a path that can also affected significantly by the gravity of a large planet. This spin-orbit resonance, as astronomers call it, would determine the length of a day on an asteroid by forcing its rotation rate to a certain value. It also controls the direction of the polar axis. More work needed "These results give us a new way to look at the asteroids," said study leader David Vokrouhlicky of Charles University in Prague. "It is our hope that this work will stimulate observational studies into many different regions of the main asteroid belt. We have only scratched the surface of this interesting problem." The study will be detailed in the Sept. 11 issue of the journal Nature. Richard Binzel, an MIT astronomer who was not involved in the research, said Slivan's findings last fall "almost defied belief." The new computer model shows promise for explaining the observations, but other asteroid families will need to be studied to prove the model out, Binzel said. "A light touch might be the best way to influence asteroid spins," Binzel writes in an accompanying Nature analysis. Received on Wed 10 Sep 2003 03:45:55 PM PDT |
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