Geodesic
Change in the Mutual Distance of Celestial Bodies Resulting From Changes in Some of Their
Publications of the Department of Astronomy, Tome 13 (1985) no. 1

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The formula developed for the distance change of two celestial bodies, resulting from the changes in the perihelia arguments, longitudes of the ascending nodes and the inclinations of their orbits. For illustration, the formula is applied to a pair of minor planets at their closest approach. 
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     author = {J. Lazovi\'c},
     title = {Change in the {Mutual} {Distance} of {Celestial} {Bodies} {Resulting} {From} {Changes} in {Some} of {Their}},
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J. Lazović. Change in the Mutual Distance of Celestial Bodies Resulting From Changes in Some of Their. Publications of the Department of Astronomy, Tome 13 (1985) no. 1. http://geodesic.mathdoc.fr/item/PDA_1985_13_1_a0/