| 21. | A particle orbiting in the Schwarzschild metric can have a stable circular orbit with.
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| 22. | First of all the typical application is a near-circular orbit.
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| 23. | For circular orbits apse line is not defined, because eccentricity is equal to zero.
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| 24. | Note that in this picture the circular orbit is approximated by straight line segments.
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| 25. | For circular orbits, the altitude is approximately 20, 200 km.
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| 26. | It travels in a low, circular orbit with a period of about 95 minutes.
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| 27. | Below we consider a circular orbit in astrodynamics or celestial mechanics under standard assumptions.
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| 28. | For circular orbits, higher orbits have a lower orbital velocity.
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| 29. | Second, assume the satellite moves in a circular orbit and it remains in synchronous rotation.
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| 30. | A star passing too close could knock a planet out of its generally circular orbit.
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