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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 ...
Coin showing Caesar's Comet as a star with eight rays, tail upward. Non-periodic comets are seen only once. ... This page was last edited on 18 April 2022, ...
Comet WISE and Comet NEOWISE may refer to any comets below discovered by the Wide-field Infrared Survey Explorer satellite between 2009 and 2024: Periodic comets
MeepCity was the first game on Roblox to pass 1 billion total visits. [61] The game was averaging 100,000 concurrent players in July 2018. [60] The game received criticism throughout 2021 due to the number of online daters inside the game and inappropriate clothing and actions found in the party feature. This caused the game to be placed as ...
C/2024 G3 (ATLAS) is a non-periodic comet, which will reach perihelion on 13 January 2025, at a distance of 0.09 AU from the Sun. It could become the brightest comet of 2025, [4] possibly exceeding apparent magnitude of −3.5. The comet is visible in the southern hemisphere before and after perihelion.
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The Taurids are an annual meteor shower, associated with the comet Encke.The Taurids are actually two separate showers, with a Southern and a Northern component. The Southern Taurids originated from Comet Encke, while the Northern Taurids originated from the asteroid 2004 TG 10, possibly a large fragment of Encke due to its similar orbital parameters.
Most sungrazing comets are part of the Kreutz family. [8] The group generally has an eccentricity approaching 1, [9] orbital inclination of 139–144° (precluding close encounters with planets), [10] a perihelion distance of less than 0.01 AU (less than the diameter of the Sun [11]), an aphelion distance of about 100 AU [12] and an orbital period of about 500–1,000 years. [4]