apoapsis oor Sweeds

apoapsis

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(astronomy) The point of a body's elliptical orbit about the system's centre of mass where the distance between the body and the centre of mass is at its maximum. For some celestial bodies, specialised terms are used: see Apsis (Wikipedia) for details.

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apoapsis

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point on an orbit furthest from the focus
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The planet's orbit stays inside the system's habitable zone for most of its revolution around the star, though at apoapsis, the planet falls outside of this zone.
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The radially integrated brightness of the ε ring is highest near apoapsis and lowest near periapsis.
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The signal looked like a strong enhancement of the forward-scattering at the wavelength 3.6 cm near ring’s apoapsis.
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The orbital eccentricity is 0.277, which means that at the separation at closest approach, or periapsis, is only 57% of the distance at their greatest separation, or apoapsis.
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Although its closest approach to the Sun is closer than Mars orbit, its highly elliptical orbit takes it almost half-way to Jupiter at its apoapsis, and as such its semi-major axis is too large for it to be classified as an Amor asteroid.
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These variations are connected with the variations of the ring width, which is 19.7 km at the periapsis and 96.4 km at the apoapsis.
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The orbit had a periapsis of 262 km (163 mi) above the northern hemisphere, and an apoapsis of 54,026 km (33,570 mi) above the southern hemisphere.
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