the sun follow the celestial sphere
The sun is always in different places at different times.
Different constellations are visible at different times of the year due to the Earth's orbit around the Sun. As the Earth moves, our nighttime view of the sky changes, revealing different stars and constellations. For instance, in winter, we see constellations that are opposite the Sun in the sky, while in summer, we see those that are closer to the Sun. This shift occurs gradually throughout the year, resulting in a dynamic night sky.
A year on each planet is determined by its orbital period around the sun. For example, a year on Earth is around 365 days, while a year on Mars is about 687 Earth days. The length of a year on a planet is influenced by its distance from the sun and its orbital speed.
Earth revolves,so we can see different parts of the night Sky as it orbits the sun
The position of the sun changes throughout the year due to the Earth's tilt, causing the sun's angle to vary, leading to different solar angles and lengths of daylight at different times of the year. This results in the changing seasons as the sun's position affects how much sunlight each hemisphere receives.
The Earth's axis is tilted.
because the world is in different places around the sun at different times of the year therefore you would see different constalations
The sun is always in different places at different times.
Stonehenge is built in a way that the sun hits different stones at different times of the year. They had to know where to line up the stones. The stones are 'aligned' with the sun. At different times of the year, the sun shines on different stones, making it like a giant sundial.
Stonehenge is built in a way that the sun hits different stones at different times of the year. They had to know where to line up the stones. The stones are 'aligned' with the sun. At different times of the year, the sun shines on different stones, making it like a giant sundial.
Energy flux (from the sun - to space) varies with the seasons.
Earth moves around the Sun. As a result, the apparent position of the Sun in the sky changes.
The tilt of the Earth's axis (approximately 23.5 degrees) and its revolution around the Sun result in varying angles of sunlight received at different times of the year. During summer in a given hemisphere, the Sun appears higher in the sky at noon, leading to increased solar intensity and longer daylight hours. Conversely, in winter, the Sun is lower in the sky, resulting in shorter days and less intense sunlight. This seasonal variation in the altitude of the midday Sun is a direct consequence of the Earth's axial tilt and its orbital position around the Sun.
because of the different weather around the world at different times of the year and how the earth and sun move
changing of the earth's axis
Earth orbiting the sun
Earth orbiting the sun