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  2. Apsis - Wikipedia

    en.wikipedia.org/wiki/Apsis

    The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1). An apsis (from Ancient Greek ἁψίς (hapsís) 'arch, vault'; pl. apsides / ˈ æ p s ɪ ˌ d iː z / AP-sih-deez) [1] [2] is the farthest or nearest point in the orbit of a planetary body about its primary body.

  3. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    The ancient Greek astronomer Hipparchus noted the apsidal precession of the Moon's orbit (as the revolution of the Moon's apogee with a period of approximately 8.85 years); [4] it is corrected for in the Antikythera Mechanism (circa 80 BCE) (with the supposed value of 8.88 years per full cycle, correct to within 0.34% of current measurements). [5]

  4. Quaoar - Wikipedia

    en.wikipedia.org/wiki/Quaoar

    The approximate perihelion (q) and aphelion (Q) dates are marked for their respective orbits. Polar view of Quaoar's orbit (yellow) along with various other large Kuiper belt objects. Quaoar orbits the Sun at an average distance of 43.7 AU (6.54 billion km; 4.06 billion mi), taking 288.8 years to complete one full orbit around the Sun.

  5. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    The Earth spends less time near perihelion and more time near aphelion. This means that the lengths of the seasons vary. [ 14 ] Perihelion currently occurs around 3 January, so the Earth's greater velocity shortens winter and autumn in the northern hemisphere, and summer and spring in the southern hemisphere.

  6. List of Solar System objects by greatest aphelion - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    An object with an e of between 0 and 1 will have an elliptical orbit, with, for instance, an object with an e of 0.5 having a perihelion twice as close to the Sun as its aphelion. As an object's e approaches 1, its orbit will be more and more elongated before, and at e =1, the object's orbit will be parabolic and unbound to the Solar System (i ...

  7. Aten asteroid - Wikipedia

    en.wikipedia.org/wiki/Aten_asteroid

    The Aten asteroid with the smallest known perihelion is also the one with the highest known eccentricity: (137924) 2000 BD 19 has an orbit with an eccentricity of 0.895, which takes it from a perihelion of 0.092 AU, well within Mercury's orbit, to an aphelion of 1.66 AU, which is greater than the semi-major axis of Mars (1.53 AU).

  8. Glossary of literary terms - Wikipedia

    en.wikipedia.org/wiki/Glossary_of_literary_terms

    Also apophthegm. A terse, pithy saying, akin to a proverb, maxim, or aphorism. aposiopesis A rhetorical device in which speech is broken off abruptly and the sentence is left unfinished. apostrophe A figure of speech in which a speaker breaks off from addressing the audience (e.g., in a play) and directs speech to a third party such as an opposing litigant or some other individual, sometimes ...

  9. File:Perihelion-Aphelion.svg - Wikipedia

    en.wikipedia.org/wiki/File:Perihelion-Aphelion.svg

    English: Shows the definition of Perihelion and Aphelion with the sun. The ellipse is exaggerated for effect, but the focus is in the correct position for the eccentricity. The ellipse is exaggerated for effect, but the focus is in the correct position for the eccentricity.