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Celestial poles

Astronomy Celestial PoleCelestial sphere

Celestial Poles
The celestial poles are the two points where the projection of the Earth's rotation axis intersects with the celestial sphere.

 


Celestial poles Points on the celestial sphere directly above the Earth's poles about which all the stars seem to rotate; known as the north and south celestial poles (NCP and SCP).

Celestial poles- the imaginary points on the sky where Earth's rotation axis, extended infinitely, would touch the imaginary celestial sphere ...

Celestial Poles The two points where Earth's axis of rotation is projected onto the celestial sphere.
Celestial Sphere The projection of space and the objects therein onto an imaginary sphere surrounding the Earth and centred on the observer.

Celestial Poles - The Earth's axis of rotation projected onto the celestial sphere. The celestial poles on the celestial sphere correspond to the North and South rotational poles on the Earth.

Celestial Poles - these are points on the Celestial Sphere that are directly above the Earth's Poles, so there is a Celestial North Pole and a Celestial South Pole.

Celestial Poles
The two points at which the Earth's axis of rotation, if extended, would intersect the celestial sphere.
Celestial Sphere ...

celestial poles - Points about which the celestial sphere appears to rotate, intersections of the celestial sphere with the earth's polar axis.

Celestial Poles
The North and South poles of the celestial sphere.
Celestial Sphere
An imaginary sphere around the Earth on which the stars and planets appear to be positioned.

CELESTIAL POLES
The celestial poles are the projection of the Earth's poles onto the celestial sphere.
CELESTIAL SPHERE
The celestial sphere is an imaginary sphere whose center is the Earth. This sphere is used by to map celestial objects.

The celestial poles have no physical relevance other than as convenient reference points for terrestial astronomy and navigation.

The celestial poles are the projections of the Earth's north and south poles into the . Because of , these poles wander along a circle with a period of about 26,000 years.

The points where Earth's rotation axis intersects the celestial sphere are called the north and south celestial poles. The line where Earth's equatorial plane cuts the celestial sphere is the celestial equator.

North and South Celestial Poles
The north ands south pivots points around which the sky appears to rotate.
Nova ...

At the equator both celestial poles are at the horizon and motion is anti-clockwise (i.e. to the left) around the North Star and clockwise (i.e to the right) around the southern celestial pole.

Halfway between the celestial poles is the celestial equator, this is a projection of the Earth's equator onto the sky. The stars on the celestial equator will rise due east and set due west.

celestial equator (NASA SP-7, 1965) The primary great circle of the celestial sphere in the equatorial system, everywhere 90° from the celestial poles; the intersection of the extended plane of the equator and the celestial sphere.

In the celestial coordinate system the North and South Celestial Poles are determined by projecting the rotation axis of the Earth to intersect the celestial sphere, which in turn defines a Celestial Equator.

To designate the position of a star, the astronomer considers an imaginary great circle passing through the celestial poles and through the star in question. This is the star's hour circle, analogous to a meridian of longitude on earth.

How do the positions of the celestial equator, celestial poles, zenith, and meridian depend on the latitude of the observer?
Would their position with respect to the horizon change if the Earth were only 200 miles in diameter?

From south to north, Theta, Beta (Menkalinan), and Delta Aurigae are in remarkable alignment almost exactly along the "solstitial colure," the great circle in the sky that connects the celestial poles with the summer and winter solstices.

First, the positions of the south and north celestial poles appear to move in circles against the space-fixed backdrop of stars, completing one circuit in 25,772 Julian years (2000 rate).

This is the slow movement of the celestial poles tracing out large circles on the celestial sphere. It is caused by a slow wobble in the Earth's axis due to the gravitational effects of the Sun and Moon on the Earth's equatorial bulge.

"one second of time"); as one moves away from the celestial equator, one must multiply this factor of 15 by an additional factor (cosine of the declination), because the lines of right ascension get closer and closer as one nears the celestial poles, ...

Another way of finding the invisible equator is to use the fact that it is 90° from the celestial poles. These too are invisible, but can be located because they are the centres of the circles traced out by the stars each day and night.

What is the great circle on the celestial sphere halfway between the celestial poles?
What connection is there between the North and South Pole and the earth's axis?
What is meant by the sigma point?
What is the equatorial coordinate system?

Like the globe in the drawing, the sphere of the sky has two points around which it turns, points that mark its axis --the celestial poles.

The projection onto the sky of the Earth's axis of rotation results in two notable points at opposite directions: the north and south celestial poles. Because of precession, these points trace out circles on the sky.

Meridian is a great circle on the celestial sphere that passes through your zenith and also through both celestial poles. Your meridian line extends all the way around the Earth (and intersects your nadir, on the other side).

An imaginary arc passing through the celestial poles and through the zenith is called the observer's meridian. The nadir is the direction opposite the zenith: for example, straight down from a spacecraft to the center of the planet.

The period of the variation of the celestial poles (about 416-433 days, with a peak at 428 days). Pole wandering (by as much as 15 meters from its mean position) causes minute variations in the meridian. [H76]
Chandra ...

For more exact measurements of time, astronomers use the meridian, which is a circle on the celestial sphere that passes both through the zenith (the point directly overhead) and both celestial poles.

celestial coordinates: a grid system for locating things in the sky. It's anchored to the celestial poles and the celestial equator (directly above Earth's equator).

Celestial pole
the north and south celestial poles are points on the celestial sphere where earths axis of rotation intersects the celestial sphere.

ecliptic ~: {celestial ~} [β, Î"] or [ELAT, ELON] the system of ecliptic (or celestial) latitude and longitude, defined with respect to the ecliptic and the celestial poles.

Diurnal motion is an astronomy term referring to the apparent daily motion of stars around the Earth, or more precisely around the two celestial poles....

The Celestial Poles lie directly above the Poles on the Earth, so if you were at the North Pole, the North Celestial Pole would be directly overhead. Keep in mind that the places on the so-called Celestial Sphere are directions not positions .

Meridian - The great circle passing through an observer's zenith and the north and south celestial poles
Mesopause - The upper boundary of the mesosphere layer of the atmosphere of a planet ...

His zenith is then in the equator and the celestial poles are in the North and South horizon respectively. The circles in which the heavenly bodies appear to revolve are then vertical.

The position of the celestial poles also changes with precession. Thus, to locate an object from its right ascension and declination, you must also know the date for which those coordinates are valid; that date is called the epoch of the coordinates.

The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles onto the celestial sphere defines the north and south celestial poles.

Each night they appear to rotate around the celestial poles due to the Earth's rotation about its axis. However, the Earth spins rather like a spinning top. Not only does the Earth rotate, it wobbles.

celestial equator the Earth's equator projected onto the sky celestial poles the Earth's north and south poles projected onto the sky comet a small body comprised of a nucleus of dirt and ice; when it nears the Sun, the ice melts, ...

See also: Celestial Pole, Earth, Sky, Equator, Circle