The seasons are due to axial tilts of planets and the apparent motion of stars and sun on the celestial sphere is due to diurnal motion.
The Sun's annual motion is from west to east relative to the fixed stars due to the Earth's orbit around the Sun. This apparent motion is caused by the Earth's revolution around the Sun, giving the illusion that the Sun is moving against the background of stars in the sky.
The motion of Earth around the Sun is the cause of the seasons.
Apparent daily motion refers to the perceived movement of celestial objects, such as the Sun and stars, across the sky over the course of a day due to the Earth's rotation on its axis. This motion gives the illusion that these objects rise in the east and set in the west. While the actual positions of these celestial bodies remain relatively fixed in space, their apparent movement is a result of our perspective from the rotating Earth.
Stars appear to move with the seasons due to the Earth's orbit around the sun. As the Earth revolves around the sun, the position of the stars we see at night changes throughout the year. This creates the illusion that stars are moving across the sky along with the changing seasons.
According to Copernicus, the Earth moved in three primary ways: it rotated on its axis daily, which accounted for the apparent movement of the stars and the sun across the sky; it orbited the sun annually, explaining the changing seasons; and it, along with other planets, revolved around the sun in a circular motion. This heliocentric model challenged the longstanding geocentric view that placed Earth at the center of the universe.
The Sun's annual motion is from west to east relative to the fixed stars due to the Earth's orbit around the Sun. This apparent motion is caused by the Earth's revolution around the Sun, giving the illusion that the Sun is moving against the background of stars in the sky.
The real motion of stars is hardly noticeable even over a period of many years. It's the Earth's daily rotation the is the main cause of their apparent motion. (Stars are so far away that the Earth's revolution around the Sun hardly cases any apparent motion.)
The apparent daily motion of the sun is from east to west due to the rotation of the Earth on its axis.
The sun's apparent path through the background of stars is called the ecliptic. It is the apparent annual path that the sun follows as seen from Earth.
A planet is said to be in retrograde motion when its apparent motion - the motion as seen by us, against the background stars - is from east to west.Planets spend more time in prograde motion, from west to east. The apparent movement of Sun and Moon against the background stars is also from west to east. Not to be confused with the daily motion, due to Earth's rotation.
Let's disregard the five visible planets right now; there isn't any simple pattern as to what seasons they are visible. For the "fixed" stars, we do not see them move. They DO move, but they are so far away that you wouldn't notice the difference in a human lifetime. As the Earth orbits the Sun, different constellations are visible from a particular location, during the year. That's because the Sun appears to move slowly around the sky during the year as we orbit the Sun. Of course, the Sun then blocks our view of the constellations near it in the sky. In fact, "circumpolar constellations" can be seen all year because they never go below the horizon. So they can be seen when the Sun isn't in the sky. An important consequence of our orbiting around the Sun is that any given star rises about four minutes earlier every night. That's because our 24 hour "solar day" is about 4 minutes longer than the Earth's rotation period. So, the stars appear to move slowly westwards in the sky during the year. Obviously, this apparent motion of the stars, relative to the Sun, is related to the seasons. The patterns of stars visible in the sky in winter are always the same. There are different patterns of stars visible in the spring, summer, or fall.
parallax :)
The motion of Earth around the Sun is the cause of the seasons.
The "ecliptic". In truth, the Sun doesn't move; the apparent motion of the Sun across the sky is caused by the Earth spinning, and the apparent motion of the Sun across the "celestial sphere" is caused by the Earth orbiting the Sun. But the plane of the Earth's orbit around the Sun is what causes the apparent motion of the Sun across the celestial sphere, so the "ecliptic" is actually the plane of the Earth's orbit.
The apparent motion of the sun is the way the sun appears to move across the sky from east to west due to the Earth's rotation. This motion creates day and night cycles. The sun reaches its highest point at noon, and its path changes throughout the year due to Earth's tilt and orbit around the sun.
Stars appear to move with the seasons due to the Earth's orbit around the sun. As the Earth revolves around the sun, the position of the stars we see at night changes throughout the year. This creates the illusion that stars are moving across the sky along with the changing seasons.
The sun rises in the east and sets in the west. This is, of course, apparent motion and not true motion.