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  2. 26P/Grigg–Skjellerup - Wikipedia

    en.wikipedia.org/wiki/26P/Grigg–Skjellerup

    Comet Grigg–Skjellerup (formally designated 26P/Grigg–Skjellerup) is a periodic comet. It was visited by the Giotto probe in July 1992. [ 6 ] The spacecraft came as close as 200 km, but could not take pictures because some instruments were damaged from its encounter with Halley's Comet . [ 7 ]

  3. de Havilland Comet - Wikipedia

    en.wikipedia.org/wiki/De_Havilland_Comet

    The last Comet 4 variant, the Comet 4C, first flew on 31 October 1959 and entered service with Mexicana in 1960. [142] The Comet 4C had the Comet 4B's longer fuselage and the longer wings and extra fuel tanks of the original Comet 4, which gave it a longer range than the 4B.

  4. Observational history of comets - Wikipedia

    en.wikipedia.org/.../Observational_history_of_comets

    The Laws of Refraction allows the human eye to visually see the tail of a comet in space at a different position than it truly is because of the reflection from the Sun. [26] Tycho Brahe's sketching of his observations of the Great Comet of 1577 in his notebook. A great comet appeared in the sky above Europe on 1577 AD.

  5. Striking photos show stunning, once-in-a-lifetime comet ... - AOL

    www.aol.com/striking-photos-show-stunning-once...

    Scientists say comet C/2023 A3 Tsuchinshan-ATLAS is visible once every 80,000 years, and people across North America were treated to stunning views. Striking photos show stunning, once-in-a ...

  6. How to Watch a Once-in-160,000-Year Comet Predicted to Shine ...

    www.aol.com/lifestyle/watch-once-160-000-comet...

    Comet G3 ATLAS (C/2024) is expected to make its return for a close encounter with the Sun in mid-January, giving skywatchers the chance to spot one of the brightest comets in 20 years from Earth.

  7. Lists of comets - Wikipedia

    en.wikipedia.org/wiki/Lists_of_comets

    Coin showing Caesar's Comet as a star with eight rays, tail upward. Non-periodic comets are seen only once. They are usually on near-parabolic orbits that will not return to the vicinity of the Sun for thousands of years, if ever.