The actual motion of stars is very hard to see because stars are very far away.
Motion
Proper motion: The apparent movement of a star across the sky due to its actual motion through space. Radial motion: Motion of a star toward or away from an observer, causing a shift in its spectral lines due to the Doppler effect. Orbital motion: Stars in binary or multiple star systems can exhibit motion around a common center of mass due to gravitational interactions.
The rotation of the Earth makes the stars appear to move in the sky.
Seasons are caused by the tilt of Earth's axis as it orbits the Sun, which creates variations in temperature and daylight. The apparent motion of the stars and the Sun is due to Earth's rotation on its axis, giving the illusion that these objects move across the sky.
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.
The apparent velocity of a star relative to another star is the speed at which one star appears to move across the sky when observed from the perspective of the other star. This apparent motion is due to the actual motion of both stars through space and can be influenced by factors such as their distance from each other and their individual velocities.
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.)
All the stars are fixed to a sphere, which rotates once in 24 hours.
the actual movement of the stars through the backdrop of other stars is one answer
A star's brightness at a standard distance is referred to as its apparent magnitude. This standard distance is 10 parsecs (32.6 light-years) from Earth. Apparent magnitude allows astronomers to compare the brightness of stars as seen from Earth, regardless of their actual distance from us.
The intrinsic motion of stars refers to their individual motion within a galaxy, which is influenced by factors such as their orbits around the galaxy's center, interactions with other stars, and their velocity relative to us on Earth. This motion is distinct from the apparent motion we observe due to the rotation of the Earth and the motion of the galaxy itself.