page_title: Comet Kohoutek
hierarchical_section_title: Comet Kohoutek
caption_attribution_description: English: This color photograph of the comet Kohoutek (C/1973 E1) was taken by members of the lunar and planetary laboratory photographic team from the University of Arizona, at the Catalina observatory with a 35mm camera on January 11, 1974.
context_page_description: Comet Kohoutek, formally designated C/1973 E1, 1973 XII, and 1973f, was first sighted on 7 March 1973 by Czech astronomer Luboš Kohoutek. It attained perihelion on 28 December that same year.
  Comet Kohoutek is a long-period comet; its previous apparition was about 150,000 years ago, and its next apparition will be in about 75,000 years. At its apparition in 1973, it had a hyperbolic trajectory due to gravitational perturbations from giant planets. Due to its path, scientists theorized that Kohoutek was an Oort-cloud object. As such, it was believed that this was the comet's first visit to the inner Solar System, which would result in a spectacular display of outgassing. Infrared and visual telescopic study have led many scientists to conclude, in retrospect, that Kohoutek is actually an Edgeworth/Kuiper-belt object, which would account for its apparent rocky makeup and lack of outgassing.
  Before its close approach, Kohoutek was promoted by the media as the "comet of the century". However, Kohoutek's display was considered a let-down, possibly due to partial disintegration when the comet closely approached the Sun prior to its Earth flyby.
context_section_description: Comet Kohoutek, formally designated C/1973 E1, 1973 XII, and 1973f, was first sighted on 7 March 1973 by Czech astronomer Luboš Kohoutek. It attained perihelion on 28 December that same year.
  Comet Kohoutek is a long-period comet; its previous apparition was about 150,000 years ago, and its next apparition will be in about 75,000 years. At its apparition in 1973, it had a hyperbolic trajectory (e > 1) due to gravitational perturbations from giant planets. Due to its path, scientists theorized that Kohoutek was an Oort-cloud object. As such, it was believed that this was the comet's first visit to the inner Solar System, which would result in a spectacular display of outgassing. Infrared and visual telescopic study have led many scientists to conclude, in retrospect, that Kohoutek is actually an Edgeworth/Kuiper-belt object, which would account for its apparent rocky makeup and lack of outgassing.
  Before its close approach, Kohoutek was promoted by the media as the "comet of the century". However, Kohoutek's display was considered a let-down, possibly due to partial disintegration when the comet closely approached the Sun prior to its Earth flyby. Since this was probably the comet's first visit to the inner Solar System, it would have still contained large amounts of frozen volatiles since its formation. Although it failed to brighten to the levels expected, it was still a naked-eye object. Its greatest visual magnitude was −3, when it was at perihelion, 0.14 AU (21,000,000 km; 13,000,000 mi) from the Sun. Its orbital inclination is 14.3°. Its best viewing was in the night sky after perihelion, when it had dimmed to fourth magnitude. The comet also sported a tail up to 25° long, along with an anti-tail.
  Kohoutek was observed by the crews of Skylab 4 and Soyuz 13; it thus became the first comet to be observed by a manned spacecraft, for Apollo 13's planned observations of the prominent naked-eye Comet Bennett had been aborted by the Moon-bound craft's oxygen-tank explosion.
  C/1973 E1 should not be confused with the periodic comet 75D/Kohoutek, which can also be called "Comet Kohoutek". In addition, there are another two long-period comets, C/1969 O1-A (a.k.a. 1970 III, 1969b), and C/1973 D1 (a.k.a. 1973 VII, 1973e) also discovered by Luboš Kohoutek.
caption: A color photograph of the comet Kohoutek
  taken on 11 January 1974.
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