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File:Apophis model comparison.png

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Marina Brozović, Lance A.M. Benner, Joseph G .McMichael, Jon D. Giorgini, Petr Pravec, Petr Scheirich, Christopher Magric, Michael W. Busch, Joseph S.Jao, Clement G.Lee, Lawrence G.Snedeker, Marc A. Silva, Martin A.Slade, Boris Semenov, Michael C. Nolan, Patrick A. Taylor, Ellen S. Howell, Kenneth J.
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Comparison between the best-fit convex and nonconvex shape models, and the available radar images of (99942) Apophis. The best-fit nonconvex model is bilobed, providing a better fit to the data.
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Adapted from Marina Brozović et al. "Goldstone and Arecibo radar observations of (99942) Apophis in 2012–2013", Icarus Volume 300, 15 January 2018, Pages 115-128; Research Data, application 1
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