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According to Carlos and Ra〓〓l de la Fuente Marcos, orbital dynamics brothers at the Complutense University of Madrid, the variance of the estimates did not provide a clear orbit to use to track sibling asteroids.〓〓 The brothers decided to run simulations of billions of possible orbits to isolate those that were likely to result in a collision.〓〓 Then, they averaged the ten best orbits and looked through a NASA asteroid catalog for objects on comparable paths.〓〓 The brothers discovered 20 such objects, which ranged from 5- to 20-meters wide.
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