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== Worst case, maximum delta-''v'' == As the example above demonstrates, the Ξ''v'' required to perform a Hohmann transfer between two circular orbits is not the greatest when the destination radius is infinite. (Escape speed is {{radic|2}} times orbital speed, so the Ξv required to escape is {{radic|2}} β 1 (41.4%) of the orbital speed.) The Ξv required is greatest (53.0% of smaller orbital speed) when the radius of the larger orbit is 15.5817... times that of the smaller orbit.<ref>{{Cite book |last=Vallado |first=David Anthony |title=Fundamentals of Astrodynamics and Applications |page=317 |publisher=Springer |date=2001 |isbn=0-7923-6903-3 |url=https://books.google.com/books?id=PJLlWzMBKjkC}}</ref> This number is the positive root of {{math|1=''x''<sup>3</sup> β 15''x''<sup>2</sup> β 9''x'' β 1 = 0}}, which is <math display="inline">5+4\,\sqrt{7}\cos\left({1\over 3}\arctan{\sqrt{3}\over 37}\right)</math>. For higher orbit ratios the {{math|Ξ''v''}} required for the second burn decreases faster than the first increases.
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