The American Ephemeris and Nautical AlmanacU.S. Government Printing Office, 1900 - Nautical almanacs |
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Common terms and phrases
Aldebaran Aldebaran E Antares Antares W Apparent Declination apparent noon APPARENT PLACES Apparent Right Ascension Aquarii Arietis Arietis E ASCENSION AND DECLINATION Besselian Cancri Capricorni CONSTANTS OF STRUVE d h m Direction of Object eclipse Ephemeris Fomalhaut Frid Geminorum GREENWICH MEAN NOON h m h m Horizontal Parallax Hour Angle II.I IIIh P. L. July June JUPITER JUPITER E Leonis Librę longitude LUNAR DISTANCES MARS Mean Solar Date Meridian Passage Midnight Minute Moon MOON'S RIGHT ASCENSION Name and Direction Octantis P. L. of Diff P. L. of P. L. Parallax Pegasi Piscium Pollux Pollux W Regulus Regulus W Right Declina Sagittarii SATURN W Semidiameter Sept sidereal Spica STRUVE AND PETERS SUN W Sun's Tauri Thur tion Ascension tion North tion sion tion South TRANSIT AT WASHINGTON Tues UPPER TRANSIT Ursa VENUS Virginis WASHINGTON MEAN ΙΟ
Popular passages
Page 508 - Sidereal Time. — Sidereal time is measured by the daily motion of the stars; or, as it is used by astronomers, by the daily motion of that point in the equator from which the true right ascension of the stars is counted.
Page 404 - In the year 1896 there will be four eclipses, two of the Sun and two of the Moon.
Page 507 - Solar time is that used for all the purposes of ordinary life, and is measured by the daily motion of the sun. A Solar Day is the interval of time between two successive transits of the sun over the same meridian; and the hour-angle of the sun is called Solar Time.
Page 508 - The civil day begins twelve hours before the astronomical day; therefore the first half of the civil day corresponds to the last half of the preceding astronomical day, and the last half of the civil day coincides with the first half of the astronomical day of the same date. Thus, January 9, 2 o'clock, AM, civil time, is January 8, 14'', astronomical time; and January 9, 2 o'clock, PM, civil time, is also January 9, 2h, astronomical time.
Page 515 - The heliocentric latitude is counted from the true ecliptic of the date The Logarithm of Radius Vector is the logarithm of the distance of the center of the planet from that of the Sun, at the Greenwich mean noon whose date is given in the first column. The last two columns give, respectively, the logarithm of the true distance of the center of the planet from that of the Earth, for the Greenwich noon indicated on the...
Page 513 - Greenwich mean time, beginning at noon; the dates are therefore astronomical. All the distances that can be observed on the same day, are grouped together under that date; and the columns are read from left to right, across both pages of the same opening. The letter W. or E. is affixed to the name of the sun, planet or star, to indicate that it is on the west, or east side of the moon. An observer on the earth's surface having...
Page 514 - Passage shows the hour, minute and tenth of that passage of the planet over the meridian of Greenwich which occurs next after the noon of the date. The right ascension and declination of a planet are required whenever it is observed for time, latitude or azimuth. The mode of reducing the...
Page 542 - CORRECTION REQUIRED, ON ACCOUNT OF SECOND DIFFERENCES OF THE MOON'S MOTION, IN FINDING THE GREENWICH TIME CORRESPONDING TO A CORRECTED LUNAR DISTANCE.
Page 143 - The semidiameter for mean noon may be assumed the same as that for apparent noon. The sign — prefixed to the hourly change of declination indicates that north declinations are decreasing or south declinations increasing. Diff. for i Hour, +9-8565'.