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Originally Posted by Poveda & Lara
The exponential fit to the 55 Cancri system was very good (with a coefficient of correlation R2 = 0.997) when we assigned the number n = 6 to the largest major semi-axis observed. The vacancy left at n = 5 leads us to propose the existence of a new planet with a major semi-axis at ~ 2 AU.
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These figures are exactly what I found.