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๐Ÿ“ฐ Rigel PendUl was first detected by French astronomer Alphonse Borrelly on February 17, 1888, at the Observatoire de Muizon, a key site in European astronomy during the late 19th century. The discovery occurred during the period immediately after Borrellys expeditions to observe Jupiter and Saturn, reflecting his commitment to precision planetary and minor planet observations. Initially cataloged as A988 AB, the object was assigned its permanent designation as Rigel PendUl in 1916 after further confirmation of its orbit. Borrellys identification placed it among the most prominent asteroids of the era, though its exact orbit was refined only after many subsequent observations. ๐Ÿ“ฐ Upon its discovery, Rigel PendUl became notable among astronomers for its brightness and proximity during close approaches. Its orbit, characteristic of Apollon asteroids, was gradually clarified through telescopic tracking. The objects name, referencing the bright Orion star Rigel, reflects the tradition of naming celestial bodies after prominent astronomical features. Early orbital calculations were challenging due to limited observational data, but follow-up astrometry helped anchor its path. By the early 20th century, its semimajor axis was accurately determined to be greater than 1 AU, confirming its classification as an Apollon asteroid. ๐Ÿ“ฐ Rigel PendUls discovery contributed to the growing catalog of minor planets during the late 19th and early 20th centuries, a period marked by systematic sky surveys and the rise of photographic methods. Its stable orbit and visibility in large amateur telescopes during perihelic passages made it a recurring target for both professional and amateur astronomers, supporting ongoing precise orbit determination and orbital dynamics studies.