south celestial pole
södra himmelspolen
celestial poles oor Sweeds
celestial poles
en
Plural form of celestial pole.
Vertalings in die woordeboek Engels - Sweeds
himmelspol
Crossing the south celestial pole are what appear to be two patches of cloud.
Nära den södra himmelspolen finns något som förefaller vara två molnfläckar.
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
Soortgelyke frases
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
Because the direction of the Earth 's spin axis changes, so does the location of the Celestial Poles
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Celestial Equator Celestial Poles Geographic Coordinate System
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Crossing the south celestial pole are what appear to be two patches of cloud.
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Celestial Poles
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The Celestial Poles
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Later, in the year 93,830 AD, Sirius will miss aligning with the south celestial pole by only 2.3 degrees.
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In the next 7500 years, the south Celestial pole will pass close to this star and Omega Carinae (5800 CE).
Blodet hade redan koaguleratWikiMatrix WikiMatrix
Despite their faintness, Gould upheld their Bayer designation as they were closer than 25 degrees to the south celestial pole.
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We said that the celestial pole is the pole of the Equatorial coordinate system. What do you think is the pole of the horizontal (Altitude/Azimuth) coordinate system? (The Zenith
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It is also the first Chinese globe that shows constellations near to the Celestial South Pole.
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There will also be periods during the cycle when bright stars give only an approximate guide to "north", as they may be greater than 5° of angular diameter removed from direct alignment with the north celestial pole.
Jag är på bronWikiMatrix WikiMatrix
The Local Meridian is an imaginary Great Circle on the Celestial Sphere that is perpendicular to the local Horizon. It passes through the North point on the Horizon, through the Celestial Pole, up to the Zenith, and through the South point on the Horizon
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While other stars might line up with the north celestial pole during the 26,000 year cycle, they do not necessarily meet the naked eye limit needed to serve as a useful indicator of north to an Earth-based observer, resulting in periods of time during the cycle when there is no clearly defined North Star.
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The North Celestial Pole currently has nearly the same coordinates as the bright star Polaris (which is Latin for Pole Star). This makes Polaris useful for navigation: not only is it always above the North point of the horizon, but its Altitude angle is always (nearly) equal to the observer 's Geographic Latitude (however, Polaris can only be seen from locations in the Northern hemisphere
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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
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From about 4300 BC until 3942 BC, it was the closest star to the celestial north pole visible to the naked eye, although it was still too dim to be regarded as a pole star.
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At the equator you see all of the celestial sphere, at either pole only one half.
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Precession is easiest to see by observing the Celestial Pole. To find the pole, first switch to Equatorial Coordinates in the Configure & kstars; window, and then hold down the Up arrow key until the display stops scrolling. The declination displayed in the center of the Info Panel should be +# degrees, and the bright star Polaris should be nearly at the center of the screen. Try slewing with the left and right arrow keys. Notice that the sky appears to rotate around the Pole
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In the late period of the Ming Dynasty, the agricultural scientist and mathematician Xu Guangqi (1562 – 1633 CE) introduced 23 additional constellations near to the Celestial South Pole, which are based on star catalogues from the West (see Matteo Ricci).
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The sky appears to drift overhead from east to west, completing a full circuit around the sky in # (Sidereal) hours. This phenomenon is due to the spinning of the Earth on its axis. The Earth 's spin axis intersects the Celestial Sphere at two points. These points are the Celestial Poles. As the Earth spins; they remain fixed in the sky, and all other points seem to rotate around them. The celestial poles are also the poles of the Equatorial Coordinate System, meaning they have Declinations of +# degrees and-# degrees (for the North and South celestial poles, respectively
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We will now demonstrate Precession by changing the Date to a very remote year, and observing that the location of the Celestial Pole is no longer near Polaris. Open the Set Time window (Ctrl; S), and set the date to the year # (currently, & kstars; cannot handle dates much more remote than this, but this date is sufficient for our purposes). Notice that the sky display is now centered at a point between the constellations Cygnus and Cepheus. Verify that this is actually the pole by slewing left and right: the sky rotates about this point; in the year #, the North celestial pole will no longer be near Polaris
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Alderamin is located near the precessional path traced across the celestial sphere by the Earth's North pole.
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In the centre is the apparently still point of the south celestial pole.
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Precession will next point the north celestial pole at stars in the northern constellation Cepheus.
Profetian IjugerParaCrawl Corpus ParaCrawl Corpus
Xingguans near southern celestial pole were created following the introdution of Western constellations into China by Catholic missionaries.
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40 sinne gevind in 11 ms. Hulle kom uit baie bronne en word nie nagegaan nie.