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单词 celestial latitude
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celestial latitude
5. Astronomy. The angular distance of a heavenly body from the ecliptic: called spec. celestial latitude. (See also ascending n., geocentric adj. 1, heliocentric adj. 1, and heliographic adj. 1)The history of this sense appears to be as follows. Originally the word was applied, on the analogy of the geographical use (see 4) to denote the angular distance of a point in the celestial sphere from the equator, measured along a secondary to the latter. This, however, was not accurately distinguished by name from the distance of a point from the ecliptic, the terms ‘latitude’ and ‘declination’ being employed indiscriminately with reference to both these ways of indicating position. (Cf. quot. c1400.) In modern use, the terms have been differentiated, declination being appropriated to what was originally and with historical propriety called ‘latitude’, while latitude became the name for distance from the ecliptic.
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the world > the universe > heavenly body > position of heavenly body > [noun] > latitude
latitudec1400
degree1647
co-latitude1790
c1400 ( G. Chaucer Treat. Astrolabe (Cambr. Dd.3.53) (1872) ii. §17. 28 Fro [the] Equinoxial may the declinacion or the latitude of any body celestial be rikned, after the site north or south,..& riht so may the latitude or the declinacion of any body celestial, saue only of the sonne..be rekned fro the Ecliptic lyne.
1556 R. Record Castle of Knowl. 176 Proprelye they doo call that the Latitude of the Planetes, when they swarue from the Ecliptike line.
1594 T. Blundeville Exercises iii. i. xi. f. 143v The Latitude is counted from the said Ecliptique line towards any of the Poles of the Zodiaque.
1601 P. Holland tr. Pliny Hist. World I. 11 Mars in his latitude leaueth the eclipticke line foure halfe degrees.
1706 Phillips's New World of Words (new ed.) (at cited word) Apparent Latitude, is the Distance of the apparent, or seeming Place of any Planet from the Ecliptick; and True Latitude is the Distance of its real Place from the same Ecliptick.
1868 J. N. Lockyer Elem. Lessons Astron. §555. 269 The right ascension and declination are then easily converted by calculation into celestial longitiude and latitude if required.
extracted from latituden.
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