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  2. C/1970 K1 (White–Ortiz–Bolelli) - Wikipedia

    en.wikipedia.org/wiki/C/1970_K1_(White–Ortiz...

    Comet White–Ortiz–Bolelli (formal designations: C/1970 K1, 1970 VI, and 1970f) was a bright comet which appeared in 1970. It was a member of the Kreutz sungrazers , [ 5 ] a family of comets which resulted from the break-up of a large parent comet several centuries ago.

  3. Comet - Wikipedia

    en.wikipedia.org/wiki/Comet

    The word comet derives from the Old English cometa from the Latin comēta or comētēs. That, in turn, is a romanization of the Greek κομήτης 'wearing long hair', and the Oxford English Dictionary notes that the term (ἀστὴρ) κομήτης already meant 'long-haired star, comet' in Greek.

  4. Technical Pan - Wikipedia

    en.wikipedia.org/wiki/Technical_Pan

    The field shown is about 6.5°x4.8°. Note the prominent disconnection event in the comet's ion tail. Stars in the image appear trailed, as the camera tracked the comet during the exposure. An unused roll of Kodak Technical Pan 35 mm film. Technical Pan is an almost panchromatic black-and-white film that was produced by Kodak. While it can ...

  5. C/1988 A1 (Liller) - Wikipedia

    en.wikipedia.org/wiki/C/1988_A1_(Liller)

    The comet reached minimum elongation on 13 March, on 25°. [4] It reached its peak brightness in April. Jacobson spotted the comet with naked eye on April 18. David H. Levy reported that the comet had an apparent magnitude of 4.7 with the naked eye on April 24. In the end of April the tail of the comet was reported to be up to 2–3 degrees long.

  6. Comet Bennett - Wikipedia

    en.wikipedia.org/wiki/Comet_Bennett

    Soon after the first orbital elements could be calculated, it was suggested that the comet would become "a bright object, that could be observed with unaided eye."It was found to combine three favorable characteristics that made it an exceptional comet for observation: a short perihelion distance, a short distance from Earth, and high intrinsic brightness. [9]

  7. C/2012 X1 (LINEAR) - Wikipedia

    en.wikipedia.org/wiki/C/2012_X1_(LINEAR)

    Comet LINEAR, formal designation C/2012 X1, is a non-periodic comet that was observed telescopically from 2012 to 2015. It produced a powerful outburst on 21 October 2013, which raised its brightness 100 times its expected magnitude from 12 to 8.5 for several months.

  8. List of comets by type - Wikipedia

    en.wikipedia.org/wiki/List_of_comets_by_type

    This is a list of comets (bodies that travel in elliptical, parabolic, and sometimes hyperbolic orbits and display a tail behind them) listed by type. Comets are sorted into four categories: periodic comets (e.g. Halley's Comet), non-periodic comets (e.g. Comet Hale–Bopp), comets with no meaningful orbit (the Great Comet of 1106), and lost comets (), displayed as either P (periodic), C (non ...

  9. Comet NEOWISE - Wikipedia

    en.wikipedia.org/wiki/Comet_NEOWISE

    Discovery image – the comet appears as three fuzzy red dots in this composite of three infrared images taken by NEOWISE on March 27, 2020. The object was discovered by a team using the WISE space telescope under the NEOWISE program on March 27, 2020. [1] It was classified as a comet on March 31 and named after NEOWISE on April 1. [5]