Elements of Astronomy ...: With Explanatory Notes, and Questions for Examination |
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Page v
... des- the heavens , cribe circles , 38 39 Circle of perpetual apparition , .. 41 Circle of perpetual occultation ,. 42 Latitude of any place equal to the elevation of the pole of 1937 595 45 vii Page . Page . Of the precession of the.
... des- the heavens , cribe circles , 38 39 Circle of perpetual apparition , .. 41 Circle of perpetual occultation ,. 42 Latitude of any place equal to the elevation of the pole of 1937 595 45 vii Page . Page . Of the precession of the.
Page vi
... Latitude and longitude ,. 53 49 The signs , 54 Zodiac ,. 54 CHAPTER IV . OF REFRACTION AND PARALLAX . Refraction , Variation of refraction in respect to altitude , .. The effect of refraction on the position of heavenly bodies ,. Its ...
... Latitude and longitude ,. 53 49 The signs , 54 Zodiac ,. 54 CHAPTER IV . OF REFRACTION AND PARALLAX . Refraction , Variation of refraction in respect to altitude , .. The effect of refraction on the position of heavenly bodies ,. Its ...
Page vii
... latitude , 98 Obliquity of the ecliptic affected Terrestrial latitude constant , 98 by nutation ,. 103 Sun's apparent diameter ,. .. 105 Anomalistic year , 107 Apparent angular motion , .. Variation in the earth's orbitual 108 Product ...
... latitude , 98 Obliquity of the ecliptic affected Terrestrial latitude constant , 98 by nutation ,. 103 Sun's apparent diameter ,. .. 105 Anomalistic year , 107 Apparent angular motion , .. Variation in the earth's orbitual 108 Product ...
Page viii
... latitude , 168 PHYSICAL ASPECTS OF THE Diurnal libration , .. 169 MOON ,. 152 Length of the lunar day , .. 169 Lunar mountains ,. 153 The appearance of the earth as The heights measured ,. 154 seen from the moon , .... ...... 170 156 ...
... latitude , 168 PHYSICAL ASPECTS OF THE Diurnal libration , .. 169 MOON ,. 152 Length of the lunar day , .. 169 Lunar mountains ,. 153 The appearance of the earth as The heights measured ,. 154 seen from the moon , .... ...... 170 156 ...
Page 26
... latitude and longitude ; these distances have been computed , and are found to be in all instances nearly equal . This fact proves the spherical shape of the earth , since a sphere alone of all solid bodies possesses the property , that ...
... latitude and longitude ; these distances have been computed , and are found to be in all instances nearly equal . This fact proves the spherical shape of the earth , since a sphere alone of all solid bodies possesses the property , that ...
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Common terms and phrases
altitude angular aphelion apogee apparent diameter apparent motion appear apsides ascertained asteroid astronomers atmosphere axis celestial equator celestial sphere centre changes circle circumference comet constellation craters degrees Describe difference direction discovered disk earth earth's orbit equal Explain from figure extent fixed stars globe Grammar heavenly body heavens hemisphere horizon hundred illumined inclination inferior conjunction J. R. Hind Jupiter latitude latter length libration longitude lunar eclipse magnitude Mars mean solar measured Mercury meridian miles moon moon's orbit mountains move nearly nebula nodes observations occur parallax passing penumbra perigee perihelion period planet position precession Prof quarter radius rays refraction respecting revolution revolve right angle right ascension ring rotation satellites Saturn seen shadow sidereal sidereal day solar day solar distance solar eclipse space spectator spots sun's surface synodical month tance telescope tides tion triangle velocity Venus vernal equinox visible west to east zenith
Popular passages
Page 296 - The fourth term is found by multiplying the second and third terms together and dividing by the first § 14O.
Page 24 - A sphere is a solid bounded by a curved surface, every point of which is equally distant from a point within called the center.
Page 164 - These phenomena do not, however, occur at every new and full moon ; and the reason is, that the plane of the moon's orbit is inclined to that of the ecliptic, and that these two planes' meet one another only in their line of common section, which passes through the centre of the earth.
Page 305 - On a careful re-examination of the heavens, too, and a comparison of catalogues, many stars are now found to be missing-; and although there is no doubt that these losses have often arisen from mistaken entries, yet in many instances it is equally certain that there is no mistake in the observation or entry, and that the star has really been observed, and as really has disappeared from the heavens...
Page 24 - A SPHERE is a solid bounded by a curved surface, every part of which is equally distant from a point within, called the centre.
Page 162 - In some of the principal ones, decisive marks of volcanic stratification, arising from successive deposits of ejected matter, and evident indications of Lava currents streaming outwards in all directions, may be clearly traced with powerful telescopes.
Page 13 - Dodd, I find it greatly superior to all others which have come under my notice, in system, completeness, and nomenclature. The arrangement is natural, the system complete, and the nomenclature greatly improved. These improvements are not slight; they are fundamental— eminently worthy the attention of the mathematical teacher, and give a character of unity to the work which at once distinguishes it from all others on this subject.
Page 50 - ... the sun. More Accurate Computations. — A more accurate determination of the phases as visible at any point of the earth's surface may be obtained from the Besselian elements which are given for every ten minutes of Greenwich mean time. Their geometric signification is as follows: — Let us imagine a plane passing through the centre of the earth, perpendicular to the right line joining the centres of the sun and moon. This latter line is the axis of the moon's shadow, and the plane is called...
Page 51 - Circles are great circles passing through the zenith of an observer, and perpendicular to his horizon. The vertical circle passing through the east and west points of the horizon is called the Prime Vertical ¡ that passing through the north and south points coincides with the celestial meridian.
Page 318 - This is an irresolvable nebula, figured by Sir John Herschel, during his residence at the Cape of Good Hope. Its favourable position, as seen in southern latitudes, enabled Herschel to trace the outline of the nebula much farther than any preceding observer had done. The singular figure of this object seems to suggest some power of attraction operating on the particles of matter, or the...