On the Connexion of the Physical SciencesJ. Murray, 1858 - 523 pages |
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... determined from it Lunar , Solar , and Planetary Eclipses - Occulta- tions and Lunar Distances Mean Distance of the Sun from the Earth obtained from Lunar Theory - Absolute Distances of the Planets , how found - - - - 34 SECTION VI ...
... determined from it Lunar , Solar , and Planetary Eclipses - Occulta- tions and Lunar Distances Mean Distance of the Sun from the Earth obtained from Lunar Theory - Absolute Distances of the Planets , how found - - - - 34 SECTION VI ...
Page 3
... every motion in the solar system has been so completely explained , that the laws of any astronomical phenomena that may hereafter occur are already determined . - SECTION I. - - Attraction of a Sphere - B 2 INTRODUCTION . 3.
... every motion in the solar system has been so completely explained , that the laws of any astronomical phenomena that may hereafter occur are already determined . - SECTION I. - - Attraction of a Sphere - B 2 INTRODUCTION . 3.
Page 10
... determination of its elliptical motion , the nature and position of its orbit must be ascertained by observation ... determine the form of the orbit ; the longitude of the planet when at its least distance from the sun , called the ...
... determination of its elliptical motion , the nature and position of its orbit must be ascertained by observation ... determine the form of the orbit ; the longitude of the planet when at its least distance from the sun , called the ...
Page 11
... determine the path of a celestial body when attracted by a second body , and disturbed in its motion round the second ... determined . It is an extremely difficult one , and would be infinitely more so if the disturbing action were not ...
... determine the path of a celestial body when attracted by a second body , and disturbed in its motion round the second ... determined . It is an extremely difficult one , and would be infinitely more so if the disturbing action were not ...
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... determined , by M. Valz , at Nimes , has a mean distance of 1.88 ; so it revolves within the zone of instability . It has a shorter periodic time than any of those previously discovered , and a greater excentricity , with the exception ...
... determined , by M. Valz , at Nimes , has a mean distance of 1.88 ; so it revolves within the zone of instability . It has a shorter periodic time than any of those previously discovered , and a greater excentricity , with the exception ...
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61 Cygni absorbed action appears atmosphere attraction bismuth blue bodies centre centrifugal force chemical circular polarization coloured rings comet consequently copper crystal dark density diamagnetic diameter diminishes direction distance disturbing earth ecliptic effect electricity equal equator ethereal medium excentricity experiments extreme force gravitation greater heat hemisphere increase intensity Jupiter latitude length lines liquid longitude luminous lunar magnetic mass mean meridian metallic miles molecules moon motion move nebula nodal lines nodes NOTE nutation observed optic axis orbit parallax paramagnetic particles passing perihelion period perpendicular phenomena plane polarized light pole position prism produced quantity rays reflected refraction refrangible retrograde motion revolution revolving right angles rotation round satellites Sir John Herschel solar spectrum sound space stars substances sun's surface telescope temperature terrestrial theory tion tourmaline transmitted tricity undulations Uranus vapour velocity vibrations violet visible Voltaic waves wire