On the Connexion of the Physical SciencesJ. Murray, 1858 - 523 pages |
From inside the book
Results 1-5 of 98
Page 14
... side of its path , and now on the other , whilst the ellipse itself is slowly , but per- petually , changing both in form and position . The periodic inequalities are merely transient deviations of a planet from its path , the most ...
... side of its path , and now on the other , whilst the ellipse itself is slowly , but per- petually , changing both in form and position . The periodic inequalities are merely transient deviations of a planet from its path , the most ...
Page 15
... side of the disturbing force . For it is clear , that if the motion be accelerated through a certain space , and then retarded through as much , the motion at the end of the time will be the same as if no change had taken place . But ...
... side of the disturbing force . For it is clear , that if the motion be accelerated through a certain space , and then retarded through as much , the motion at the end of the time will be the same as if no change had taken place . But ...
Page 18
... side of the disturbing force , the average motion of these points , after a revolution of the disturbed body , is retrograde , and comparatively rapid : but , when the disturbing planet is so situated that the orbit of the disturbed ...
... side of the disturbing force , the average motion of these points , after a revolution of the disturbed body , is retrograde , and comparatively rapid : but , when the disturbing planet is so situated that the orbit of the disturbed ...
Page 21
... side of the small planets , is 4546 miles , and that of the earth 7925 miles , so that the telescopic group are too minute to disturb the others . M. Le Verrier found another zone of instability between Venus and the sun , on the border ...
... side of the small planets , is 4546 miles , and that of the earth 7925 miles , so that the telescopic group are too minute to disturb the others . M. Le Verrier found another zone of instability between Venus and the sun , on the border ...
Page 25
... side of the sun , and all three in the same straight line , they are then said to be in conjunction ( N. 83 ) . Now , if they begin to move at the same time , one making exactly five revolutions in its orbit while the other only ...
... side of the sun , and all three in the same straight line , they are then said to be in conjunction ( N. 83 ) . Now , if they begin to move at the same time , one making exactly five revolutions in its orbit while the other only ...
Other editions - View all
Common terms and phrases
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