On the Connexion of the Physical Sciences |
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Page ix
Elliptical Motion — Mean and True Motion -- Equinoctial — Ecliptic - Equinoxes — Mean and True Longitude - Equation of Centre - Inclination of the Orbits of Planets Celestial Latitude Nodes — Elements of an Orbit — Undisturbed or ...
Elliptical Motion — Mean and True Motion -- Equinoctial — Ecliptic - Equinoxes — Mean and True Longitude - Equation of Centre - Inclination of the Orbits of Planets Celestial Latitude Nodes — Elements of an Orbit — Undisturbed or ...
Page 8
Elliptical Motion - Mean and True Motion · Equinoctial Ecliptic Equinoxes Mean and True Longitude Equation of Centre — Inclination of the Orbits of Planets - Celestial Latitude Nodes Elements of an Orbit — Undisturbed or Elliptical ...
Elliptical Motion - Mean and True Motion · Equinoctial Ecliptic Equinoxes Mean and True Longitude Equation of Centre — Inclination of the Orbits of Planets - Celestial Latitude Nodes Elements of an Orbit — Undisturbed or Elliptical ...
Page 9
The equinoctial , which is a great circle traced in the starry heavens by the imaginary extension of the plane of the terrestrial equator , is intersected by the ecliptic , or apparent path of the sun , in two points diametrically ...
The equinoctial , which is a great circle traced in the starry heavens by the imaginary extension of the plane of the terrestrial equator , is intersected by the ecliptic , or apparent path of the sun , in two points diametrically ...
Page 10
The orbits of the recently - discovered planets deviate more from the ecliptic than those of the ancient planets : that of Pallas , for instance , has an inclination of 34 ° 42 29.8 " to it ; on which account it is more difficult to ...
The orbits of the recently - discovered planets deviate more from the ecliptic than those of the ancient planets : that of Pallas , for instance , has an inclination of 34 ° 42 29.8 " to it ; on which account it is more difficult to ...
Page 13
... 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 and of the Universe Great Inequality of Jupiter and Saturn .
... 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 and of the Universe Great Inequality of Jupiter and Saturn .
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Contents
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absorbed according action angle appears atmosphere attraction axis becomes bismuth blue bodies cause centre chemical colour comet consequently continually crystal dark depends determined diameter diminishes direction distance disturbing earth ecliptic effect electricity equal equator ether exist experiments extends extreme fall force give glass gravitation greater green heat increase instance intensity John known latitude length less light lines liquid magnetic mass matter mean measured medium metallic miles moon motion move nature nearly NOTE object observed opposite orbit particles passing periodic phenomena plane plate polarized pole position produced proportion proved quantity rays reflected refraction refrangible revolving rings rotation round satellites seen separated shows side similar solar sound space spectrum square stars substances surface temperature theory tion transmitted undulations varies vibrations visible waves whole wire