stellar parallax oor Spaans
stellar parallax
en
the heliocentric parallax of a star
Vertalings in die woordeboek Engels - Spaans
Paralaje estelar
en
apparent shift of position of a nearby star against the background of distant objects during Earth's orbital period
That difference, that angular difference, is the stellar parallax.
Esa diferencia, esa diferencia angular, es el paralaje estelar.
paralaje estelar
That difference, that angular difference, is the stellar parallax.
Esa diferencia, esa diferencia angular, es el paralaje estelar.
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voorbeelde
Advanced filtering
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The stellar parallax therefore, is very small and actually very hard to detect.
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The greatest of these was the absence of stellar parallax.
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It wasn't until the 19th century that scientists were able to detect the stellar parallax.
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That difference, that angular difference, is the stellar parallax.
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Astronomers looked for the stellar parallax and they found nothing, nothing at all.
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He made the first measurement of stellar parallax: 0.3 arcsec for the binary star 61 Cygni.
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And so this slide here illustrates a concept known as stellar parallax.
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The nearest star system, ALPHA CENTAURI, has a stellar parallax of 0.76 second of arc.
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He became well known for his work on stellar parallaxes and photometry.
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Then, from 1952-1955 he was the president of Commission 24, the Stellar Parallaxes section, of the International Astronomical Union.
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From 1899 to 1903, he was an astronomer at Yerkes, where he pioneered the use of photographic methods to determine stellar parallaxes.
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Research at the observatory over the years includes stellar parallaxes, stellar statistics, galactic structure, external galaxies, stellar atmospheres and solar system research.
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As a result of his work the knowledge of stellar parallaxes for the southern hemisphere became better known than that of the northern.
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Starting in 1914 the second director, Samuel Alfred Mitchell, began a program to measure the distances to nearby stars (stellar parallax) using photography.
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Distances to the very closest stars, those within 200 light-years or so, can be measured directly by stellar parallax, which involves simple trigonometry.
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Because the stars were actually much further away than Greek astronomers postulated (making movement extremely subtle), stellar parallax was not detected until the 19th century.
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It contradicted not only empirical observation, due to the absence of an observable stellar parallax, but more significantly at the time, the authority of Aristotle.
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It was first observed in the late 1600s by astronomers searching for stellar parallax in order to confirm the heliocentric model of the Solar System.
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First of all, if the Earth did move, then one ought to be able to observe the shifting of the fixed stars due to stellar parallax.
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In 1720, James Bradley carried out a series of experiments attempting to measure stellar parallax by taking measurements of stars at different times of the year.
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Being very difficult to measure, only about 60 stellar parallaxes had been obtained by the end of the 19th century, mostly by use of the filar micrometer.
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Most of Jackson’s time at the Cape was taken up with the determination of stellar parallax, a programme that had been started by his predecessor, Harold Spencer Jones.
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Frank Schlesinger first demonstrated the technique of determining stellar parallaxes photographically at Yerkes in 1905, and Mitchell (along with Frederick Slocum) carried out research applying the technique, publishing their results in 1913.
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This assumption can also be expressed by saying that the stellar parallax caused by the motion of the Earth around its orbit equals the solar parallax caused by motion around the Earth.
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In 1952 John Jackson was awarded The Gold Medal of the Royal Astronomical Society for his work on stellar parallaxes and his contributions to the general problems of star positions and proper motions.
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68 sinne gevind in 14 ms. Hulle kom uit baie bronne en word nie nagegaan nie.