celestial latitude oor Spaans
celestial latitude
en
(astronomy) the angular distance of a celestial body north or to the south of the celestial equator; expressed in degrees; used with right ascension to specify positions on the celestial sphere
Vertalings in die woordeboek Engels - Spaans
declinación
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Vertoon algoritmies gegenereerde vertalings
voorbeelde
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Voorbeelde moet herlaai word.
In this essay, however, we’re concerned only with celestial latitude, which is a good break for us.
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Every star can be said to be at some particular celestial latitude.
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That means their celestial latitude does not change with time.
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We call celestial latitude declination.
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Bradley’s Star Catalogue gives the Declination, or Celestial Latitude, for each Star.
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Not only does Ptolemy give the position of a star in celestial longitude and latitude but he adds more detail.
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I n middle-northern latitudes the celestial pole is approximately 45° above the northernmost point on the horizon.
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And once we have a celestial equator, we can measure the latitude of a star.
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The greater the latitude, the higher the celestial Pole will be in the sky.
Déjala a ellaLiterature Literature
The plates were etched with latitudes, altitudes, even parts of the celestial sphere.
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Stars on the celestial equator are not circumpolar when observed from any latitude in either hemisphere of the Earth.
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Nevertheless, the device was thought to be some kind of astrolabe, an instrument once commonly used to determine latitude by the positions of celestial bodies.
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And what this shows us is that his zenith is, at any given time, going to be at a declination, a distance from the celestial equator also equal to his latitude.
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Latitude with Polaris and upper meridian transit of any celestial body are also included.
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If the observer's latitude is 35° S, then all stars within 35° of the south celestial pole are circumpolar.
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Islamic geography and navigational sciences were highly developed, making use of a magnetic compass and a rudimentary instrument known as a kamal, used for celestial navigation and for measuring the altitudes and latitudes of the stars.
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The position of a star on the celestial sphere can only be perfectly known with a system of three co-ordinates: the celestial longitude brought back to an origin, the celestial latitude and the distance.
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For observers at moderate latitudes, who can see the sky near the celestial pole of their hemisphere better than that nearer the horizon, this may be a good reason to prefer a planisphere made with the polar azimuthal equidistant projection method.
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And, now as the Earth rotates we observe if you want as the celestial sphere rotates from east to west, the star will move along this line of latitude.
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For example, if the observer's latitude is 50° N, any star will be circumpolar if it is less than 50° from the north celestial pole.
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These two diameters have a 90 degree angle between them, the net result is that this angle here is also the observer's latitude which means, remembering that this is the horizon, that your latitude is the angle from the horizon to whichever celestial pole is visible.
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A circumpolar star is a star, as viewed from a given latitude on Earth, that never sets below the horizon due to its apparent proximity to one of the celestial poles.
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Declination is to a celestial globe as latitude is to a terrestrial globe, a vertical positioning of an object.
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Depending on the observer's latitude on Earth, some stars – the circumpolar ones – are close enough to the celestial pole to remain continuously above the horizon, while other stars dip below the horizon for some portion of their daily circular path (and others remain permanently below the horizon).
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The Ecliptic coordinate system uses the Ecliptic for its Fundamental Plane. The Ecliptic is the path that the Sun appears to follow across the sky over the course of a year. It is also the projection of the Earth 's orbital plane onto the Celestial Sphere. The latitudinal angle is called the Ecliptic Latitude, and the longitudinal angle is called the Ecliptic Longitude. Like Right Ascension in the Equatorial system, the zeropoint of the Ecliptic Longitude is the Vernal Equinox
Bélgica informará a la Comisión, en un plazo de dos meses a partir de la notificación de la presente Decisión, de las medidas adoptadas en cumplimiento de la mismaKDE40.1 KDE40.1
57 sinne gevind in 10 ms. Hulle kom uit baie bronne en word nie nagegaan nie.