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Gamma Normides is considered one of the weak meteor showers, as it produces 6 meteors per hour, and is active annually from February 25 to March 28, and its peak occurs from March 13 to March 15 each year.
The Jeddah Astronomical Society has revealed that the “Gamma Normids” meteors occur within the boundaries of the constellation Norma, which is a small constellation seen in the southern hemisphere and that there will be an opportunity to see meteors. from anywhere in the world when the meteor origin point is high above the horizon near Norma’s brightest star.
In conjunction with the peak of the “Gamma Normids” meteor, the moon will be in the crescent phase at the beginning of the month, which will leave the sky dark, and the best time for surveillance will be after midnight, and after that it will remain active until. ‘at dawn, and for best results, the observation should be done from a dark, open place away from pollution Photosynthesis (not from the house) is monitored with the naked eye by observing the southern horizon without need to use binoculars or telescopes, as their fields of view are very narrow for meteors.
Meteors are likely to be at their best shortly before dawn, when their radiation is at their highest, but in most Arab cities they will stay low, close to the horizon.
In general, meteor showers occur when the Earth passes through debris scattered by comets and asteroids, and over time pieces of pebble-like debris are distributed in clusters along the orbit of the Earth. original bodies around the solar system and are seen as a strip of light. when it collides with Earth’s atmosphere, typically burning at a height of between 70 and 100 kilometers.
During certain days of the year, Earth’s orbit passes through dense debris associated with comets or asteroids that spew large amounts of solid material into space, leading to meteor showers that follow reproduce each year when the Earth passes a certain point in its orbit where it passes through certain debris.
Meteors associated with meteor showers in particular can be distinguished from others because their path appears to radiate outward from a common point in the sky, indicating the direction from which they originated. This is because the gravel particles in the given debris move in almost exactly same direction when they cross Earth’s orbit, and hit Earth in roughly the same direction and at the same speed.
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