Вопрос задан 27.08.2018 в 07:48. Предмет История. Спрашивает Смирнов Дмитрий.

Наблюдение изменений положения солнца на небе; восход и заход,видимое движение солнца по небосводу

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Отвечает Алексеева Светлана.
Солнцк движетсч , из за того что время суток меняется
Весь день оно то поднимаетсч тто опускается
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Отвечает нейросеть ChatGpt. Будьте внимательны, ответы нейросети могут содержать ошибочные или выдуманные данные.

Observing Changes in the Position of the Sun in the Sky

Observing the changes in the position of the Sun in the sky involves noting the sunrise and sunset times as well as the apparent movement of the Sun across the celestial sphere.

Sunrise and Sunset: The Sun rises in the east and sets in the west, creating the illusion of movement across the sky. The exact times of sunrise and sunset vary depending on the observer's location and the time of year. These times can be easily obtained from various sources, including weather websites, smartphone apps, or astronomical almanacs.

Apparent Movement of the Sun: The Sun appears to move across the sky due to the rotation of the Earth on its axis. This movement is from east to west, and the Sun's path is called the ecliptic. Throughout the day, the Sun gradually changes its position in relation to the observer, moving higher or lower in the sky. This apparent movement is a result of the Earth's axial tilt and its orbit around the Sun.

During the course of a day, the Sun reaches its highest point in the sky, known as the culmination or solar noon. At this point, the Sun is directly overhead for observers located on the Tropic of Cancer (23.5 degrees north latitude) on the summer solstice and the Tropic of Capricorn (23.5 degrees south latitude) on the winter solstice. For observers at other latitudes, the Sun's position at solar noon will be lower or higher in the sky, depending on their location and the time of year.

Throughout the year, the Sun's apparent path across the sky changes due to the tilt of the Earth's axis. This creates the changing seasons as the Sun's rays strike the Earth at different angles. In the Northern Hemisphere, the Sun appears higher in the sky during the summer months and lower during the winter months. The opposite is true for the Southern Hemisphere.

Conclusion

Observing the changes in the position of the Sun in the sky involves noting the times of sunrise and sunset as well as the apparent movement of the Sun across the celestial sphere. The Sun rises in the east and sets in the west, and its position in the sky changes throughout the day. The Sun's apparent movement is a result of the Earth's rotation on its axis and its orbit around the Sun. The changing position of the Sun in the sky creates the illusion of movement and is responsible for the changing seasons.

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