Elements of Astronomy: Descriptive and Physical ... |
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Page 35
... March , but the nearest fixed star is too re- mote to have that 190 millions of miles , make any apparent change in its direction , and such change would be perceptible , if the star were not more than 200 thousand times the distance of ...
... March , but the nearest fixed star is too re- mote to have that 190 millions of miles , make any apparent change in its direction , and such change would be perceptible , if the star were not more than 200 thousand times the distance of ...
Page 37
... March , but the nearest fixed star is too re- mote to have that 190 millions of miles , make any apparent change in its direction , and such change would be perceptible , if the star were not more than 200 thousand times the distance of ...
... March , but the nearest fixed star is too re- mote to have that 190 millions of miles , make any apparent change in its direction , and such change would be perceptible , if the star were not more than 200 thousand times the distance of ...
Page 42
... March , or the 23d of September , let a Quadrant be used at noon , to determine how high the Sun appears above the horizon . If found to be 48 ° , ( which is called its altitude , ) above the horizon , subtract the 48 ° , from 90 ...
... March , or the 23d of September , let a Quadrant be used at noon , to determine how high the Sun appears above the horizon . If found to be 48 ° , ( which is called its altitude , ) above the horizon , subtract the 48 ° , from 90 ...
Page 44
... March , or the 23d of September , let a Quadrant be used at noon , to determine how high the Sun appears above the horizon . If found to be 48 ° , ( which is called its altitude , ) above the horizon , subtract the 48 ° , from 90 ...
... March , or the 23d of September , let a Quadrant be used at noon , to determine how high the Sun appears above the horizon . If found to be 48 ° , ( which is called its altitude , ) above the horizon , subtract the 48 ° , from 90 ...
Page 55
... March 8 7 48 PM 1850 1851 July 13 2 8 AM July 28 8 11 AM 1852 Jan. 7 3 AM Total . Dec. 26 A M Begins 6h . 28m . What day and hour in 1831 will there be an annular eclipse ? Where ? When will there be another total solar eclipse in the ...
... March 8 7 48 PM 1850 1851 July 13 2 8 AM July 28 8 11 AM 1852 Jan. 7 3 AM Total . Dec. 26 A M Begins 6h . 28m . What day and hour in 1831 will there be an annular eclipse ? Where ? When will there be another total solar eclipse in the ...
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Common terms and phrases
24 hours 95 millions ABERRATION OF LIGHT altitude angle annular annular eclipse aphelion apparent diameter Aries Astronomy atmosphere attraction axis brass meridian called celestial centre century circle comets constellations degrees density disc Dominical letter double stars east elevated equal Equator estimated fixed stars given place heavenly bodies heavens Herschel horizon illustrate Jupiter Latitude Longitude luminary luminous lunar eclipses magnitude material worlds mean distance Mercury miles the hour millions of miles minutes Moon Moon's motion nearest nodes observation opposite orbit organs of vision parallax perihelion period planets polar pole primary refraction revolution revolves round right ascension rings rising rotation round the Earth round the Sun satellites Saturn set the index solar eclipse solstice southern hemisphere Sun's place supposed surface telescope thousand miles tides tion torrid zone transit of Venus true place turn the globe twilight velocity vernal equinox visible Zodiac
Popular passages
Page 121 - The works of the LORD are great, sought out of all them that have pleasure therein.
Page 136 - Behold I have given you every herb bearing seed, which is upon the face of all the earth, and every tree in the which is the fruit of a tree yielding seed, to you it shall be for meat.
Page 103 - Hitherto shalt thou come and no farther, and here shall thy proud waves be stayed.
Page 2 - BBOWN, of the said district, hath deposited in this office the title of a book, the right whereof he claims as author, in the words following, to wit : " Sertorius : or, the Roman Patriot.
Page 61 - evidence of things not seen," in the fulness of Divine grace ; and was profound on this, the greatest concern of human life, while unable even to comprehend how the " inclination of the earth's axis to the plane of its orbit" could be the cause of the change of the seasons.
Page 115 - Rectify the globe to the latitude of the place; bring the sun's place in the ecliptic to the meridian, and set the index to XII.
Page 104 - These are thy glorious Works, Parent of good, Almighty! thine this universal frame, Thus wondrous fair: thyself how wondrous then, Unspeakable! who sitt'st above these heavens To us invisible, or dimly seen In these thy lowest works; yet these declare Thy goodness beyond thought, and power divine.
Page 138 - Who by searching can find out God ; who can find out the Almighty to perfection...
Page 80 - The squares of the periods of revolution of any two planets are proportional to the cubes of their mean distances from the sun.
Page 65 - ... angles. In northern Latitudes, the smallest angle made by the Ecliptic and horizon, is when Aries rises, at which time Libra sets ; the greatest, when Libra rises, at which time Aries sets.