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| | chapter 24 |
 | | These bodies are massive enough for tidal effects to modify their orbits from the typical large semimajor axis, retrograde orbit characteristic of the smaller, presumably captured satellites shown in the diagram. |
 | | The retrograde lunar capture orbit contracts due to tidal dissipation until resonance between the lunar orbital period and the spin period of the Earth locks the Moon in a slowly expanding orbit. |
 | | In the latter case it is possible that such material, distributed in the Earth's orbit, caused collisional perturbation of the Moon's precapture orbit, thereby contributing to the capture of the Moon (Kaula and Harris, 1973; Kaula, 1974; Wood and Mittler, 1974; Opik, 1972). |
| www.hq.nasa.gov /pao/History/SP-345/ch24.htm (5600 words) |
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