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109P/Swift-Tuttle

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109P/Swift-Tuttle

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Swift discovered or co-discovered a number of comets, including periodic comets 11P/Tempel-Swift-LINEAR, 64P/Swift-Gehrels, and 109P/Swift-Tuttle (parent body of the Perseids meteor shower).
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1862: 109P/SwiftTuttle, the comet generating the Perseid meteor shower, was independently discovered by Lewis Swift on 16 July 1862, and by Horace Parnell Tuttle on 19 July 1862.
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Perseids - from Comet 109P Swift-Tuttle
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109P/Swift-Tuttle – Wikipedia, wolna encyklopedia
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Associated Comet: 109P/Swift-Tuttle (comet discovered in 1862)
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We can thank the comet, 109P/Swift-Tuttle, for this meteor shower which lost part of its mass on its path around the Sun.
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The apparent origin of this stream lies in the eponymous constellation Perseus; however, it consists of the decomposition products of comet 109P / Swift-Tuttle.
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We have the comet 109P/Swift-Tuttle to thank for this meteor shower, which lost part of its mass on its orbit around the Sun.
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Sin The Perseids are the traces of a comet, 109P / Swift -Tuttle that the Earth in its traslation movement around the sun every year through a populated area with the fragments that leaves the comet every 133 [...]
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The highest Perseid meteor rates this year are expected to occur on from Sunday night into Monday morning August 12–13, when the Earth will be the closest to the core orbit of comet 109P/Swift-Tuttle and its debris trail.
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The highest Perseid meteor rates this year are expected to occur on from Monday night into Tuesday morning August 12-13, when the Earth will be closest to the orbit of comet 109P/Swift-Tuttle and densest part of its debris trail.
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It takes place as result of the cosmic dust leaving the tail of the comet 109P/Swift-Tuttle (I won't rememeber this name in five minutes... hehe) but this phenomenon name (St Lawrence's tears) carts, as could not be otherwise, a legend .
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The derived orbits allow to associate the meteoroids to several streams associated to comets 55P/Tempel-Tuttle, 109P/Swift-Tuttle, 3P/Encke and also one from the asteroid Phaeton. The second part is dedicated to meteor spectroscopy. Fifteen spectra obtained from the Ondrejov Observatory (Czech Republic) have been analysed.
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13 sinne gevind in 7 ms. Hulle kom uit baie bronne en word nie nagegaan nie.