On the accuracy of approximation of a small celestial body motion using intermediate perturbed orbits calculated from two position vectors and three observations.
| Autor: | Shefer, V.1 shefer@niipmm.tsu.ru, Shefer, O.2 |
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| Zdroj: | Solar System Research. Jan2015, Vol. 49 Issue 1, p51-60. 10p. |
| Databáze: | Academic Search Ultimate |
| Externí odkaz: |
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