Приклади вживання South celestial pole Англійська мовою та їх переклад на Українською
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The South Celestial Pole.
The third imaginary corner will be the south celestial pole.
South Celestial Poles.
Finding the south celestial pole.
The south celestial pole is visible only from the southern hemisphere.
This point is 5 or 6 degrees from the south celestial pole.
The South Celestial Pole does indeed exist.
Make an equilateral triangle, the third point of which is the south celestial pole.
The height of the North or South Celestial Poles exactly matches your latitude.
In addition,the constellation-free zone is not centered exactly on the south celestial pole.
The north and south celestial poles and their relation to axis of rotation, plane of orbit and axial tilt.
A flat earth model with the northpole at the centre just doesn't have any south celestial pole at all!
The south celestial pole can be located from the Southern Cross and its two"pointer" stars α Centauri and β Centauri.
In the Southern Hemisphere, stars appear to spin around the south celestial pole(but there is no bright“south star.”).
The closest equivalent is a constellationcalled the Southern Cross that rotates tightly around the south celestial pole.
Series of shots where you cansee the rotation of the Earth's axis relative to the south celestial pole, clearly see the Magellanic Clouds and the Southern Cross.
Over the years, astronomers have added constellations to fill in the gaps between Ptolemy's figures andmap the uncharted regions of the sky near the south celestial pole.
The north and south celestial poles appear permanently directly overhead to an observer at the Earth's North Pole and South Pole respectively.
However, if the earth is a spinning sphere, the velocity of the stars will begin to decline past the Celestial Equator until they stop moving at what we will call the South Celestial Pole.
If the South Celestial Pole exists, our people in these two places should be able to see it, and it should be closer to the southern horizon for our Brisbane people.
As on Earth, the effect of precession causes the north and south celestial poles to move in a very large circle, but on Mars the cycle is 171,000 Earth years.
The celestial poles are also the poles of the celestial equatorial coordinate system, meaning they have declinations of +90 degrees and-90 degrees(for the north and south celestial poles, respectively).
T\t The large group of clusters and nebulae near the south celestial pole\t\t\tare objects in the Large Magellanic Cloud, which is a dwarf galaxy in\t\t\torbit around the Milky Way.\t\t \t.
The Equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the most closely related to the Geographic coordinate system, because they use the same fundamental plane, and the same poles. 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.
As on Earth, the effect of precession causes the north and south celestial poles to move in a very large circle, but on Mars the cycle is 171,000 Earth years[19] rather than 26,000 years as on Earth.
But in reality, people in both South Africa and Western Australia, which are six hours apart, looking due south will both see the south celestial pole, and with good eyes or binoculars will see Sigma Octantis aka Polaris Australis.
The South celestial pole is correspondingly found at 9h 10m 42s and- 52° 53.0′, which is a couple of degrees from the 2.5-magnitude star Kappa Velorum(which is at 9h 22m 06.85s- 55° 00.6′), which could therefore be considered the southern polar star.
The first clue is thatAratus' constellations did not include any near the south celestial pole(the point on the celestial sphere directly above the Earth's south pole) because that area of the sky was always below the horizon of the ancient constellation-makers.
To determine the direction of the south(southern celestial pole), use the star pointers to the left of the cross.