Pereonids

The Perseids is an annual meteor shower that occurs in the Northern Hemisphere, typically between July 17 and August 24, with the peak activity occurring around August 9-13. The shower is caused by the Earth passing through the debris left behind by the comet Swift-Tuttle. The meteors appear to radiate from the constellation Perseus, hence the name "Perseids."

The Perseids are known for their high rate of meteors, with up to 100 meteors per hour during the peak. The meteors are fast-moving, with speeds of up to 60 kilometers per second, and they often leave persistent trains, which are glowing trails of ionized gas that can last for several seconds.

The Perseids are visible from both the Northern and Southern Hemispheres, although they are more visible from the Northern Hemisphere. The best time to view the shower is during the pre-dawn hours, when the radiant point is highest in the sky. The meteors can be seen with the naked eye, and no special equipment is needed.

The Perseids have been observed for over 2,000 years, with the first recorded sighting dating back to 36 AD. The shower has been the subject of many studies and observations, and it continues to be a popular target for amateur and professional astronomers alike. The Perseids are a reminder of the beauty and wonder of the night sky, and they continue to captivate and inspire people around the world.