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12 hours 24 hours according added answering apparent altitude APPARENT DISTANCE apply astronomical called centre Chronometer Constellation Corr corresponding declination deduced diff difference dist Divide effect Equation estimated EXAMPLE exceeds feet find the Error fixed Star gaining give given greater Greenwich Half Sum height horary angle horizon horizontal parallax index error interval June Latitude less LOGARITHMS Longitude lower limb manner mean meridian method Midnight minutes Moon's Nautical Almanac nearest nearly necessary noon object observed altitude observed distance observed east place of observation Polar Distance Pole Star PROBLEM proper PROPORTIONAL LOGARITHMS reduced refraction right ascension RULE Second CORRECTIONS semid semidiameter Sextant Ship slow for mean Star's subtracted Sun's Table taken telescope third correction true altitude true distance tude variation vertical watch ܗ ܗ
Page 44 - C, as seen above, are constants, depending upon the latitude of the place of observation and the declination of the star. Tables for these quantities will be found in an appendix to Annual Report US Coast and Geodetic Survey for 1874.
Page 5 - ... will be the right ascension of the meridian. From the right ascension of the meridian (increased by 24 hours if necessary) subtract the sun's right ascension...
Page 17 - Subtract the true altitude of the sun's centre from 90°, and the remainder will be the sun's true meridian zenith distance, which is to be called north or south according as the observer is north or south of the sun at the time of observation.
Page 12 - The Hare The Great Dog The Little Dog The Ship The Hydra The Cup The Crow The Centaur The Wolf The Altar The Southern Crown The Southern Fish Cuntellatnm.
Page 8 - ... distance of a heavenly body from the moon. 1. Under the given distance put down the two computed distances of the same heavenly body found in the Nautical Almanac between which the given true distance lies. 2. Take the difference between the first and second, and also between the second and the third. 3. From the proportional logarithm of the first difference subtract the proportional logarithm of the second difference, the sum is the proportional logarithm of the additional time to be added...
Page 16 - Benetnach, the Star in the point of the tail of the Great Bear, and Deneb, in the tail of the Lion, is a.