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It looks like this notation came ultimately from Forest Ray Moulton's text An Introduction to Celestial Mechanics (chapter 5, 2nd rev. ed., 1914.) He analyzes the two-body problem and defines constants of the motion ci, i=1, ..., 4. c1 is proportional to the total angular momentum of the system, and c2 fixes the origin of the time axis. Dmoews (talk) 17:47, 21 December 2024 (UTC)[reply]