The Elements of Astronomy: Designed for the Use of Students in the UniversityJ. Smith, and sold by J. Deighton and J. Nicholson, 1811 - 297 |
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... Mean Motion of the Planets XIII . On the greatest Equation , Excentricity , and Place of the Aphelia of the Orbits of the Planets 1 XIV . On the Nodes and Inclinations of the Orbits of 1 10 32 37 45 50 61 65 71 74 83 86 89 the Planets ...
... Mean Motion of the Planets XIII . On the greatest Equation , Excentricity , and Place of the Aphelia of the Orbits of the Planets 1 XIV . On the Nodes and Inclinations of the Orbits of 1 10 32 37 45 50 61 65 71 74 83 86 89 the Planets ...
Strona 8
... mean noon is 12 o'clock , by a clock adjusted to go 24 hours in a mean solar day . 56. The equation of time at noon is the interval between true and apparent noon . 57. A star is said to rise or set cosmically when it rises or sets at ...
... mean noon is 12 o'clock , by a clock adjusted to go 24 hours in a mean solar day . 56. The equation of time at noon is the interval between true and apparent noon . 57. A star is said to rise or set cosmically when it rises or sets at ...
Strona 9
... mean anomaly ; this is sometimes called the prosthapheresis . 67. Nonagesimal degree of the ecliptic is that point which is highest above the horizon . 68. The mean place of a body is the place where a body ( not moving with a uniformly ...
... mean anomaly ; this is sometimes called the prosthapheresis . 67. Nonagesimal degree of the ecliptic is that point which is highest above the horizon . 68. The mean place of a body is the place where a body ( not moving with a uniformly ...
Strona 15
... mean length of a day at every place is 12 hours . Hence , at every place , the sun , in the course of a year , is half a year above and half a year below the horizont . It is manifest , also , that the days increase from the time the ...
... mean length of a day at every place is 12 hours . Hence , at every place , the sun , in the course of a year , is half a year above and half a year below the horizont . It is manifest , also , that the days increase from the time the ...
Strona 31
... mean of the whole number of meridians so taken be drawn , the meridian may be found with sufficient accuracy for all common purposes * . 109. To find whether a wall be full south for a vertical south dial , erect a gnomon ...
... mean of the whole number of meridians so taken be drawn , the meridian may be found with sufficient accuracy for all common purposes * . 109. To find whether a wall be full south for a vertical south dial , erect a gnomon ...
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aberration aphelion apogee apparent place appear astronomers atmosphere axis called Cassini centre circle clock comet computed conjunction consequently dark declination described determined diameter difference disc discovered diurnal motion draw earth eclipse emersion equal equinox excentricity fixed stars Flamstead gives greater Halley happen heavenly bodies heavens hence Trig Herschel horary motion horizon horizontal parallax hour angle inclination inferior conjunction interval Jupiter latitude libration light lunar magnitude Mars mean anomaly mean distance mean motion Mercury meridian altitude moon moon's orbit nearly node observed opposition orbit parallax parallel perihelion perpendicular phænomena Phil planet pole proper motion radius refraction revolve right ascension ring rotation satellite Saturn seen semidiameter shadow sidereal sine solar spectator spots sun and moon sun's supposed surface synodic revolution telescope tion Trans transit triangle true anomaly true longitude true place tude umbra Venus visible zenith
Popularne fragmenty
Strona 151 - Object would not be the same when the Eye is at Rest, as when it is moving in any other Direction, than that of the Line passing through the Eye and Object; and that, when the Eye is moving in different Directions, the apparent Place of the Object would be different.
Strona 141 - ... the squares of the periodic times are as the cubes of the distances from the common centre, the centripetal forces will be inversely as the squares of the distances.
Strona 6 - The Latitude of a star is its angular distance from the ecliptic measured on a circle of latitude.
Strona 180 - ... and therefore there is a greater probability of seeing a lunar than a solar eclipse. Since the moon is as long above the horizon as below, every spectator may expect to see half the number of lunar eclipses which happen.
Strona 217 - Observer' at a salary of 100£ per annum, his duty being 'forthwith to apply himself with the most exact care and diligence to the rectifying the tables of the motions of the heavens and the places of the fixed stars, so as to find out the so much desired longitude of places for the perfecting the art of navigation.
Strona 118 - ... it had a degree of brightness about as strong as that with which such a coal would be seen to glow in faint daylight.
Strona 204 - He further observes, that there are some additional circumstances in the appearance of extended clusters and nebula-, that very much favour the idea of a power lodged in the brightest part. For, although the form of them be not globular, it is plainly to be seen that there is a tendency towards sphericity, by the swell of the dimensions...
Strona 205 - ... in diameter. The star is perfectly in the centre, and the atmosphere is so diluted, faint, and equal throughout, that there can be no surmise of its consisting of stars ; nor can there be a doubt of the evident connection between the atmosphere and the star.
Strona 40 - The Equation of Time is computed by taking the Difference of the Sun's true right Ascension and his mean Longitude corrected by the Equation of the Equinoxes in right Ascension, and turning it into Time at the Rate of 1
Strona 72 - That the planets all move in elliptic orbits, of which the sun occupies one of the foci. 3. That the squares of the times of the revolutions of the planets are as the cubes of their mean distances from the sun.