On the Connexion of the Physical SciencesJ. Murray, 1858 - 523 pages |
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Page 24
... equator of the solar system , dividing it into two parts , which balance one another in all their motions . This plane of greatest inertia , by no means peculiar to the solar sys- tem , but existing in every system of bodies submitted ...
... equator of the solar system , dividing it into two parts , which balance one another in all their motions . This plane of greatest inertia , by no means peculiar to the solar sys- tem , but existing in every system of bodies submitted ...
Page 27
... equator must soon have given the circular form observed in the orbits of the first and second satellites , which its superior attraction will always maintain . The third and fourth satellites , being farther removed from its influence ...
... equator must soon have given the circular form observed in the orbits of the first and second satellites , which its superior attraction will always maintain . The third and fourth satellites , being farther removed from its influence ...
Page 28
... equator and of the satellites . In fact , if the satellites moved exactly in the plane of Jupiter's equator , they would not be pulled out of that plane , because his attraction would be equal on both sides of it . But , as their orbits ...
... equator and of the satellites . In fact , if the satellites moved exactly in the plane of Jupiter's equator , they would not be pulled out of that plane , because his attraction would be equal on both sides of it . But , as their orbits ...
Page 29
... equator , also affect these small bodies ( N. 90 ) . The plane of Jupiter's equator is inclined to the plane of his orbit at an angle of 3 ° 5 ' 30 " , so that the action of the sun and of the satellites themselves produces a nutation ...
... equator , also affect these small bodies ( N. 90 ) . The plane of Jupiter's equator is inclined to the plane of his orbit at an angle of 3 ° 5 ' 30 " , so that the action of the sun and of the satellites themselves produces a nutation ...
Page 30
... equator , which has a very small inclination to his orbit , that the first three are eclipsed at each revolution by the shadow of the planet , which is much larger than the shadow of the moon : the fourth satellite is not eclipsed so ...
... equator , which has a very small inclination to his orbit , that the first three are eclipsed at each revolution by the shadow of the planet , which is much larger than the shadow of the moon : the fourth satellite is not eclipsed so ...
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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