On the Connexion of the Physical SciencesJ. Murray, 1858 - 523 pages |
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Page ix
... Latitude Elements of an Orbit Undisturbed or Elliptical Orbits clination of the Orbits of the New Planets Universal Gravitation the Cause of Perturbations in the Motions of the Heavenly Bodies Problem of the Three Bodies - Stability of ...
... Latitude Elements of an Orbit Undisturbed or Elliptical Orbits clination of the Orbits of the New Planets Universal Gravitation the Cause of Perturbations in the Motions of the Heavenly Bodies Problem of the Three Bodies - Stability of ...
Page 4
... latitude ( N. 13 ) , or part of the earth intermediate between the pole and the equator , where the attraction of the earth on bodies at its surface is the same as if it were a sphere ; and experience shows that bodies there fall ...
... latitude ( N. 13 ) , or part of the earth intermediate between the pole and the equator , where the attraction of the earth on bodies at its surface is the same as if it were a sphere ; and experience shows that bodies there fall ...
Page 8
... Latitude Undisturbed or Elliptical Orbits - - - Nodes Great In- clination of the Orbits of the New Planets Universal Gravitation the Cause of Perturbations in the Motions of the Heavenly Bodies - Problem of the Three Bodies Stability of ...
... Latitude Undisturbed or Elliptical Orbits - - - Nodes Great In- clination of the Orbits of the New Planets Universal Gravitation the Cause of Perturbations in the Motions of the Heavenly Bodies - Problem of the Three Bodies Stability of ...
Page 9
... latitude ( N. 54 ) , which is south or north according as the planet is south or north of that plane . When the planet is in the plane of the ecliptic , its latitude is zero ; it is then said to be in its nodes ( N. 55 ) . The ascending ...
... latitude ( N. 54 ) , which is south or north according as the planet is south or north of that plane . When the planet is in the plane of the ecliptic , its latitude is zero ; it is then said to be in its nodes ( N. 55 ) . The ascending ...
Page 13
... Latitude , and Secular Variations in the Position of the Orbit with regard to the Plane of the Ecliptic Mean Motion and Major Axis Invariable Stability of System Effects of a Resisting Medium - ― - - Invariable Plane of the Solar System ...
... Latitude , and Secular Variations in the Position of the Orbit with regard to the Plane of the Ecliptic Mean Motion and Major Axis Invariable Stability of System Effects of a Resisting Medium - ― - - Invariable Plane of the Solar System ...
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61 Cygni action appears atmosphere attraction bismuth bodies cause centre centrifugal force chemical colour comet consequently copper crystal dark degree density diamagnetic diameter diminishes direction disturbing double stars earth ecliptic effect electricity equal equator ethereal medium excentricity Fcap force glass gravitation greater heat hemisphere increase intensity Jupiter latitude length light lines liquid longitude luminous lunar magnetic major axis mass meridian metallic miles moon motion move nearly nebula nodal lines nodes northern hemisphere NOTE nutation observed optic axis orbit oscillations parallax paramagnetic particles passing perihelion periodic phenomena planets plate polarized pole position Post 8vo produced quantity rays reflected refraction refrangible revolution revolving right angles rings rotation round satellites Sir John Herschel solar spectrum space stars substances sun's surface telescope temperature terrestrial tion tourmaline transmitted tricity undulations Uranus vapour variation velocity vibrations Vols Voltaic waves wire Woodcuts