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| | Comet Encke and Taurid Meteors |
 | | In 1940 Whipple discovered that the Taurid meteors were fragments of Comet Encke, with period 3.3 years, perihelion 0.34 AU, and aphelion 4.1 AU, and that the differences in the orbits of the meteors and Comet Encke looked like the result of 14,000 years of perturbations by Jupiter. |
 | | In 1950, Whipple and Hamid discovered that the orbits of four Taurid meteors coincided with the orbit of Comet Encke as of 4700 years ago, and that, as of 1500 years ago, the orbits of three other Taurid meteors coincided with each other but not with the orbit of Comet Encke. |
 | | Clube says that fragments of Comet Encke make up the Taurid meteor stream, which peaks around 30 June in daylight hours but is visible in the night skies of November, and that the Earth passes through each dense part of this belt of debris every 3000 years. |
| www.valdostamuseum.org /hamsmith/encke.html (880 words) |
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