(Non-)detection of a quadratic drift in mean anomaly of the satellite of 1996 FG3

Physics

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Scientific paper

We present an analysis of photometric observations of binary Near-Earth asteroid (175706) 1996 FG3, observed from 1996 to 2011. The analysis gave two possible solutions for a quadratic drift of mean anomaly of the satellite, (0.0 +0.12/-0.2 deg/yr2 and ~ 12 deg/yr2. We expect to resolve between the two solutions, and to further constrain the uncertainty, using new observations obtained during 2011.

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