celestial equator oor Masedonies
celestial equator
en
A great circle on the celestial sphere, coincident with the plane of earth's equator.
Vertalings in die woordeboek Engels - Masedonies
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voorbeelde
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The ecliptic intersects the celestial equator at about 23.5 degrees.
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Points north of the celestial equator have positive declinations, while those south have negative declinations.
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As the observer moves north (or south), the celestial equator tilts towards the opposite horizon.
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Some examples of great circles on the celestial sphere include the celestial horizon, the celestial equator, and the ecliptic.
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At the moment of each equinox, the center of the Sun appears to pass through the celestial equator, and δ☉ is 0°.
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Then consider a second fictitious Sun travelling along the celestial equator at a constant speed and coinciding with the first fictitious Sun at the equinoxes.
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For example, the Sun is north of the celestial equator for about 185 days of each year, and south of it for about 180 days.
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The moment the Sun crosses the celestial equator and equalizes night and day is calculated exactly every year and Iranian families gather together to observe the rituals.
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In June and December when the sun is farthest from the celestial equator a given shift along the ecliptic corresponds to a large shift at the equator.
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In astronomy, hour angle is defined as the angular distance on the celestial sphere measured westward along the celestial equator from the meridian to the hour circle passing through a point.
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The minor irregularities of the apparent solar day were smoothed by measuring time using the mean solar day, using the Sun's movement along the celestial equator rather than along the ecliptic.
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Second, due to Earth's axial tilt (known as the obliquity of the ecliptic), the Sun's annual motion is along a great circle (the ecliptic) that is tilted to Earth's celestial equator.
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At all latitudes, the celestial equator is a uniform arc or circle because the observer is only finitely far from the plane of the celestial equator, but infinitely far from the celestial equator itself.
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The celestial equator is defined to be infinitely distant (since it is on the celestial sphere); thus, the ends of the semicircle always intersect the horizon due east and due west, regardless of the observer's position on Earth.
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The effect of this is that a clock running at a constant rate – e.g. completing the same number of pendulum swings in each hour – cannot follow the actual Sun; instead it follows an imaginary "mean Sun" that moves along the celestial equator at a constant rate that matches the real Sun's average rate over the year.
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Ordinary differential equations appear in celestial mechanics (planets, stars and galaxies); numerical linear algebra is important for data analysis; stochastic differential equations and Markov chains are essential in simulating living cells for medicine and biology.
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As seen from the Equator, the two celestial poles are on the horizon due north and south, and the motion is counterclockwise (i.e. leftward) around Polaris and clockwise (i.e. rightward) around Sigma Octantis.
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A few years after publishing The Lord of the Rings, in a note associated with the unique narrative story "Athrabeth Finrod ah Andreth" (which is said to occur in Beleriand during the War of the Jewels), Tolkien equated Arda with the Solar System; because Arda by this point consisted of more than one heavenly body (Valinor being another planet and the Sun and Moon being celestial objects in their own right and not objects orbiting the Earth).
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18 sinne gevind in 2 ms. Hulle kom uit baie bronne en word nie nagegaan nie.