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  2. Halley's Comet - Wikipedia

    en.wikipedia.org/wiki/Halley's_Comet

    Semi-major axis. 17.737 au: Eccentricity: 0.96658: Orbital period (sidereal) ... Halley's Comet is the only known short-period comet that is consistently visible to ...

  3. Great January Comet of 1910 - Wikipedia

    en.wikipedia.org/wiki/Great_January_Comet_of_1910

    The Great January Comet of 1910, formally designated C/1910 A1 and often referred to as the Daylight Comet, [2] was a comet which appeared in January 1910. It was already visible to the naked eye when it was first noticed, and many people independently "discovered" the comet.

  4. Orbital eccentricity - Wikipedia

    en.wikipedia.org/wiki/Orbital_eccentricity

    For elliptical orbits it can also be calculated from the periapsis and apoapsis since = and = (+), where a is the length of the semi-major axis. = + = / / + = + where: r a is the radius at apoapsis (also "apofocus", "aphelion", "apogee"), i.e., the farthest distance of the orbit to the center of mass of the system, which is a focus of the ellipse.

  5. 177P/Barnard - Wikipedia

    en.wikipedia.org/wiki/177P/Barnard

    Comet 177P/Barnard, also known as Barnard 2, is a periodic comet with an orbital period of 122 years. It fits the classical definition of a Halley-type comet with (20 years < period < 200 years). [4] It orbits near the ecliptic plane and has aphelion near the Kuiper cliff at 48 AU (7.2 billion km).

  6. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    Also shown are: semi-major axis a, semi-minor axis b and semi-latus rectum p; center of ellipse and its two foci marked by large dots. For θ = 0°, r = r min and for θ = 180°, r = r max. Mathematically, an ellipse can be represented by the formula: = + ⁡,

  7. Newton's theorem of revolving orbits - Wikipedia

    en.wikipedia.org/wiki/Newton's_theorem_of...

    Newton also applied his theorem to the planet Mercury, [26] which has an eccentricity ε of roughly 0.21, and suggested that it may pertain to Halley's comet, whose orbit has an eccentricity of roughly 0.97. [25] A qualitative justification for this extrapolation of his method has been suggested by Valluri, Wilson and Harper. [25]

  8. Elliptic orbit - Wikipedia

    en.wikipedia.org/wiki/Elliptic_orbit

    is the length of the semi-major axis. Conclusions: The orbital period is equal to that for a circular orbit with the orbital radius equal to the semi-major axis (), For a given semi-major axis the orbital period does not depend on the eccentricity (See also: Kepler's third law).

  9. List of long-period comets - Wikipedia

    en.wikipedia.org/wiki/List_of_long-period_comets

    For comets with an orbital period of over 1000 years (semi-major axis greater than ~100 AU), see the List of near-parabolic comets. Comet designation Name / discoverer(s)