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Libros Libros 1 - 9 de 9 sobre ... equal to 215 times the radius of the earth, which explains the difference in...
" ... equal to 215 times the radius of the earth, which explains the difference in the statements of the distance. This distance having been ascertained with tolerable accuracy, we possess the measure of our whole planetary system, as, according to the... "
Essays on Various Subjects: To which is Prefixed a Life of the Author - Página 188
por George Walker - 1809
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Encyclopaedia Americana: A Popular Dictionary of Arts, Sciences ..., Volumen12

Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford - 1832
...our whole planetary system, as, according to the second • law of Kepler (qv), the cubes of the mean distances of the planets from the sun are as the squares of the periods of their revolutions (which have long been known). Therefore the determining of this distance...
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encyclopedia americana

FRANCIS LIEBER - 1832
...cf our whole planetary system, as, according to the second law of Kepler (qv), the cubes of the mean distances of the planets from the sun are as the squares of the periods of their revolutions (which have long been known). Therefore the determining of this distance...
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Encyclopædia Americana: A Popular Dictionary of Arts, Sciences ..., Volumen12

Francis Lieber, Edward Wigglesworth - 1835
...of our whole planetary system, as, according to the second law of Kepler (qv), the cubes of the mean distances of the planets from the sun are as the squares of the periods of their revolutions (which have long been known). Therefore the determining of this distance...
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An exposition of the nature, force, action, and other properties of ...

Joseph Denison - 1842 - 40 páginas
...discovered by Kepler in the beginning of the seventeenth century, viz., that the cubes of the mean distances of the planets from the Sun are as the squares of their periodic times, is found to be invariably consistent with observation, and is therefore so firmly established,...
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Text-book of arithmetic, for the use of teachers

John Hunter (of Uxbridge.) - 1847
...264. Kepler's Third Law. Newton demonstrated the law ascertained by Kepler, that the cubes of the mean distances of the planets from the Sun are as the squares of their times of revolution. Examp. If the Earth's mean distance from the Sun be 95071447 miles, and its sidereal...
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ENCYCLOPAEDIA AMERICANA:, AMERICAN BIOGRAPHY

FRANCIS LIEBER - 1851
...of our whole planetary system, as, according to the second law of Kepler (qv), the cubes of the mean distances of the planets from the sun are as the squares of the periods of their revolutions (which have long been known). Therefore the determining of 'this distance...
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SPHERICAL ASTRONOMY

F. BRUNNOW - 1865
...the sun can be found by means of the third law of Kepler, according to which the cubes of the mean distances of the planets from the sun are as the squares of the times of revolution. Thus from this determination the parallax of the sun was found equal to 9"....
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Newton's Principia, First Book, Sections I., II., III.: With Notes and ...

Isaac Newton, Percival Frost - 1878 - 292 páginas
...each others orbits, the statement of Kepler's third law should be amended to " The cubes of the mean distances of the planets from the sun are as the squares of the periodic times multiplied into the sum of the masses of the sun and the planet. 13. Prove that,...
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Newtons Principia: Book 1, Sections 1. 2. 3 ; with Notes and Illustr. and a ...

Sir Isaac Newton, Percival Frost - 1900 - 292 páginas
...each others orbits, the statement of Kepler's third law should be amended to " The cubes of the mean distances of the planets from the sun are as the squares of the periodic times multiplied into the sum of the masses of the sun and the planet. 13. Prove that,...
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