| 11. | The greater the orbital energy, the bigger the orbit,
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| 12. | For elliptic and hyperbolic orbits } }, where " ? " is the specific orbital energy.
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| 13. | Relativity predicts that over time a binary system's orbital energy will be converted to gravitational radiation.
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| 14. | An object has reached escape velocity when the specific orbital energy is greater or equal to zero.
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| 15. | Ab initio and semi-empirical calculations yield orbital energies; therefore, they can be applied to band structure calculations.
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| 16. | As a result, Jupiter lost orbital energy, and its circuit around the sun shrank by about 2 percent.
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| 17. | Aircraft-specific energy is very similar to specific orbital energy except that it is expressed as a positive quantity.
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| 18. | This can be shown in showing specific orbital energy, through changing orbits by applying thrust throughout the series.
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| 19. | Conversely, for a given total mass and semi-major axis, the total specific orbital energy is always the same.
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| 20. | Although most metals have higher orbitals, overlap of orbital energies and crystal form ) are involved as well.
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