pylacroix
Perséides 2013
Les Perséides ou « Larmes de saint Laurent » sont une pluie d'étoiles filantes visible dans l'atmosphère terrestre, issue de débris aussi gros qu'un grain de sable de la comète Swift-Tuttle. Bien que les premières traces d'observation datent de l'an 36, ce n'est qu'entre 1864 et 1866 qu'il est établit une relation entre les Perséides et la comète dont la pluie d'étoiles filantes est issue. Ces météores sont observables lorsque les débris de Swift-Tuttle rencontrent l'atmosphère terrestre, soit à partir du 20 juillet environ jusqu'aux alentours du 25 août, avec un maximum habituellement situé entre le 11 et 13 août. C'est l'essaim le plus spectaculaire et le plus populaire de l'année, étant donné qu'il se produit, pour l'hémisphère nord, lors de la période estivale.
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The Perseids are a prolific meteor shower associated with the comet Swift-Tuttle. The Perseids are so-called because the point from which they appear to come, called the radiant, lies in the constellation Perseus. The name derives in part from the word Perseides, a term found in Greek mythology referring to the sons of Perseus.
The stream of debris is called the Perseid cloud and stretches along the orbit of the comet Swift-Tuttle. The cloud consists of particles ejected by the comet as it travels on its 133-year orbit. Most of the particles have been part of the cloud for around a thousand years. However, there is also a relatively young filament of dust in the stream that was pulled off the comet in 1865. The rate of meteors originating from this filament is much higher than for the older part of the stream.
The Perseid meteor shower has been observed for about 2,000 years, with the earliest information on this meteor shower coming from the Far East. Some Catholics refer to the Perseids as the "tears of St. Lawrence", since 10 August is the date of that saint's martyrdom.
The shower is visible from mid-July each year, with the peak in activity being between 9 and 14 August, depending on the particular location of the stream. During the peak, the rate of meteors reaches 60 or more per hour. They can be seen all across the sky, but because of the path of Swift-Tuttle's orbit, Perseids are primarily visible in the northern hemisphere. As with all meteor showers, the rate is greatest in the pre-dawn hours, since the side of the Earth nearest to turning into the sun scoops up more meteors as the Earth moves through space. Most Perseids disappear while at heights above 80 kilometres (50 mi).
Perséides 2013
Les Perséides ou « Larmes de saint Laurent » sont une pluie d'étoiles filantes visible dans l'atmosphère terrestre, issue de débris aussi gros qu'un grain de sable de la comète Swift-Tuttle. Bien que les premières traces d'observation datent de l'an 36, ce n'est qu'entre 1864 et 1866 qu'il est établit une relation entre les Perséides et la comète dont la pluie d'étoiles filantes est issue. Ces météores sont observables lorsque les débris de Swift-Tuttle rencontrent l'atmosphère terrestre, soit à partir du 20 juillet environ jusqu'aux alentours du 25 août, avec un maximum habituellement situé entre le 11 et 13 août. C'est l'essaim le plus spectaculaire et le plus populaire de l'année, étant donné qu'il se produit, pour l'hémisphère nord, lors de la période estivale.
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The Perseids are a prolific meteor shower associated with the comet Swift-Tuttle. The Perseids are so-called because the point from which they appear to come, called the radiant, lies in the constellation Perseus. The name derives in part from the word Perseides, a term found in Greek mythology referring to the sons of Perseus.
The stream of debris is called the Perseid cloud and stretches along the orbit of the comet Swift-Tuttle. The cloud consists of particles ejected by the comet as it travels on its 133-year orbit. Most of the particles have been part of the cloud for around a thousand years. However, there is also a relatively young filament of dust in the stream that was pulled off the comet in 1865. The rate of meteors originating from this filament is much higher than for the older part of the stream.
The Perseid meteor shower has been observed for about 2,000 years, with the earliest information on this meteor shower coming from the Far East. Some Catholics refer to the Perseids as the "tears of St. Lawrence", since 10 August is the date of that saint's martyrdom.
The shower is visible from mid-July each year, with the peak in activity being between 9 and 14 August, depending on the particular location of the stream. During the peak, the rate of meteors reaches 60 or more per hour. They can be seen all across the sky, but because of the path of Swift-Tuttle's orbit, Perseids are primarily visible in the northern hemisphere. As with all meteor showers, the rate is greatest in the pre-dawn hours, since the side of the Earth nearest to turning into the sun scoops up more meteors as the Earth moves through space. Most Perseids disappear while at heights above 80 kilometres (50 mi).