by neufer » Mon Aug 10, 2020 1:21 pm
https://en.wikipedia.org/wiki/Comet_Swift%E2%80%93Tuttle wrote:
<<Comet Swift–Tuttle is a large [i.e., comet nucleus 26 km in diameter] periodic comet that is in a 1:11 orbital resonance with Jupiter. It fits the classical definition of a Halley-type comet with a period between 20 and 200 years. It was independently discovered by Lewis Swift on July 16, 1862 and by Horace Parnell Tuttle on July 19, 1862. After the 1862 observations it was thought that the comet would return between 1979 and 1983, but it didn't show up. However, it had been suggested in 1902 that this was the same comet as that observed by Ignatius Kegler on July 3, 1737, and on this basis Brian Marsden calculated that it would return only in 1992, which in fact it did.
Chinese records indicate that, in 188, the comet reached apparent magnitude 0.1. Observation was also recorded in 69 BC, and it was probably visible to the naked eye in 322 BC. In the discovery year of 1862, the comet was as bright as Polaris. The comet made a return appearance in 1992, when it was rediscovered by Japanese astronomer Tsuruhiko Kiuchi and became visible with binoculars. In 2126 it will be a bright naked-eye comet reaching about apparent magnitude 0.7.
The comet's perihelion is just under that of Earth, while its aphelion is just over that of Pluto. An unusual aspect of its orbit is that it was recently captured into a 1:11 orbital resonance with Jupiter; it completes one orbit for every 11 of Jupiter. It was the first comet in a retrograde orbit to be found in a resonance. In principle this would mean that its proper long-term average period would be 130.48 years, as it librates about the resonance. Over the short term, between epochs 1737–2126 the orbital period varies between 128 and 136 years. However, it only entered this resonance about 1000 years ago, and will probably exit the resonance in several thousand years.>>
[quote=https://en.wikipedia.org/wiki/Comet_Swift%E2%80%93Tuttle]
[float=right][img3="Incomin!"]https://upload.wikimedia.org/wikipedia/commons/e/e6/Animation_of_109P%EF%BC%8FSwift%E2%80%93Tuttle_orbit.gif[/img3][/float]
<<Comet Swift–Tuttle is a large [i.e., comet nucleus 26 km in diameter] periodic comet that is in a 1:11 orbital resonance with Jupiter. It fits the classical definition of a Halley-type comet with a period between 20 and 200 years. It was independently discovered by Lewis Swift on July 16, 1862 and by Horace Parnell Tuttle on July 19, 1862. After the 1862 observations it was thought that the comet would return between 1979 and 1983, but it didn't show up. However, it had been suggested in 1902 that this was the same comet as that observed by Ignatius Kegler on July 3, 1737, and on this basis Brian Marsden calculated that it would return only in 1992, which in fact it did.
Chinese records indicate that, in 188, the comet reached apparent magnitude 0.1. Observation was also recorded in 69 BC, and it was probably visible to the naked eye in 322 BC. In the discovery year of 1862, the comet was as bright as Polaris. The comet made a return appearance in 1992, when it was rediscovered by Japanese astronomer Tsuruhiko Kiuchi and became visible with binoculars. In 2126 it will be a bright naked-eye comet reaching about apparent magnitude 0.7.
The comet's perihelion is just under that of Earth, while its aphelion is just over that of Pluto. An unusual aspect of its orbit is that it was recently captured into a 1:11 orbital resonance with Jupiter; it completes one orbit for every 11 of Jupiter. It was the first comet in a retrograde orbit to be found in a resonance. In principle this would mean that its proper long-term average period would be 130.48 years, as it librates about the resonance. Over the short term, between epochs 1737–2126 the orbital period varies between 128 and 136 years. However, it only entered this resonance about 1000 years ago, and will probably exit the resonance in several thousand years.>> [/quote]