It's because the Earth's axis is tilted. Therefore the plane of the equator is tilted (at about 23.5 degrees) away from the plane of the Earth's orbit.
Therefore the celestial equator is tilted away from the ecliptic.
The angle between the equinoctial and the ecliptic is known as the obliquity of the ecliptic. It is the angle between the plane of Earth's orbit around the Sun and the plane of the celestial equator. Currently, the obliquity of the ecliptic is about 23.5 degrees.
The celestial equator is the imaginary line in the heavens that runs around the Earth midway between the celestial poles. It is an extension of Earth's equator onto the celestial sphere and divides the sky into northern and southern hemispheres.
The celestial sphere is an imaginary sphere surrounding the Earth, with celestial equator and celestial poles located on it. The celestial equator is an extension of Earth's equator onto the celestial sphere, while the celestial poles are the points where Earth's rotation axis intersects the celestial sphere. These features can be observed in the night sky.
The imaginary extension of Earth's equator into space is called the celestial equator. It is an imaginary line in the sky above the Earth's equator, dividing the celestial sphere into northern and southern hemispheres.
An imaginary line in the middle of the sky is called the celestial equator. It is an extension of the Earth's equator into space and divides the sky into northern and southern hemispheres. This line is important in astronomy for coordinates and locating celestial objects.
The tilt of the Earth's axis (about 23.5 degrees) causes the ecliptic plane (the path the Sun appears to take through the sky) to be inclined with respect to the celestial equator. This tilt leads to the changing seasons as the Earth orbits the Sun and causes the ecliptic and celestial equator to intersect at two points, known as the equinoxes.
The celestial line that is a product of Earth's rotation is the celestial equator. It is an imaginary line located above Earth's equator and is created as a result of Earth's rotation on its axis. It divides the celestial sphere into northern and southern hemispheres.
The angle between the equinoctial and the ecliptic is known as the obliquity of the ecliptic. It is the angle between the plane of Earth's orbit around the Sun and the plane of the celestial equator. Currently, the obliquity of the ecliptic is about 23.5 degrees.
The plane of Earth's orbit is known as the ecliptic. It is the flat plane in space that represents the path along which the Earth travels around the Sun. The ecliptic is inclined at an angle of approximately 23.5 degrees to the celestial equator.
The celestial equator is the imaginary line in the heavens that runs around the Earth midway between the celestial poles. It is an extension of Earth's equator onto the celestial sphere and divides the sky into northern and southern hemispheres.
The celestial line created by Earth's revolution around the sun is called the ecliptic. This is the apparent path that the sun appears to follow across the sky over the course of a year.
The path taken by the Sun through the stars over the course of a year is called the ecliptic. This is the apparent annual path of the Sun in the sky as seen from Earth, due to the Earth's orbit around the Sun. The path of the ecliptic also marks the plane of the solar system.
In the northern hemisphere, the ecliptic is highest in the sky during the summer solstice and lowest during the winter solstice. It runs roughly east to west and is responsible for the path the Sun appears to take across the sky throughout the year.
If Earth did not rotate, the celestial poles would align with the geographic poles, and the celestial equator would align with Earth's equator. The celestial poles are points in the sky that the Earth's axis points towards, and the celestial equator is an imaginary line in the sky directly above the Earth's equator. Without Earth's rotation, these references would be fixed in the sky.
About 23.5 degrees.The celestial equator and the ecliptic are two "great circles" on the sky coordinate system.Think of them as two hoops of the same size, hinged together at two points (well the hinged points do move but very slowly taking about 26 000 years to move around and come back to the same place again). If you hold onesteady and spin the other one inside it, they stay connected at the two hinges, but they canbe set at any angle to each other.Now put them in the sky. Place the steady one right above the equator all the way around, and tiltthe movable one on the hinges so that it makes an angle of 23.5 degrees with the steady one.The steady one, above the earth's equator all the way around, is the celestial equator. The movable one,tilted 23.5 degrees to the equator, is the ecliptic ... the path that the sun appears to travel in the sky,once around in a year. The hinges ... where the ecliptic crosses the equator ... are the points where thesun is located at the time of the two equinoxes. Halfway between the hinges are the points where thetwo circles are farthest apart ... one where the ecliptic is farthest above the equator, the other whereit's farthest below. Those are the points where the sun is located at the time of the two solstices.
The celestial sphere is an imaginary sphere surrounding the Earth, with celestial equator and celestial poles located on it. The celestial equator is an extension of Earth's equator onto the celestial sphere, while the celestial poles are the points where Earth's rotation axis intersects the celestial sphere. These features can be observed in the night sky.
The equator makes an angle of roughly 23.5 degrees with the ecliptic plane.