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" ... to the inclination of the axis of the earth to the plane of the ecliptic, and partly to the different positions in which a spectator is placed in different zones of the globe. "
Lectures on Experimental Philosophy, Astronomy, and Chemistry: Intended ... - Page 1
by George Gregory - 1820
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Universal Geography: Or, A Description of All Parts of the World, on a New ...

Conrad Malte-Brun - Atlases - 1829 - 552 pages
...such, the sphere would appear parallel. As the limits of the zones and of the climates depend upon the inclination of the axis of the earth to the plane of the ecliptic, it is of importance to determine this inclination. We may easily discover it by observing at one and...
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Encyclopaedia Americana: A Popular Dictionary of Arts, Sciences ..., Volume 5

Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford - Encyclopedias and dictionaries - 1831 - 650 pages
...what manner the changes of the seasons, the increase and decrease of the days, &c., are caused by the inclination of the axis of the earth to the plane of the ecliptic, at an angle of 664 degrees, and how the axis, gy remaining parallel to itself in all points of its...
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Encyclopædia Americana: A Popular Dictionary of Arts, Sciences ..., Volume 11

Francis Lieber, Edward Wigglesworth, Thomas Gamaliel Bradford, Henry Vethake - Encyclopedias and dictionaries - 1832 - 628 pages
...time than at others, so that the solar days cannot be equal. Auother circumstance, dependent upon the inclination of the axis of the earth to the plane of the ecliptic, is also tobe taken into the account. The apparent solar time, therefore, is distinguished from mean...
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Encyclopædia Americana, ed. by F. Lieber assisted by E. Wigglesworth (and T ...

Encyclopaedia Americana - 1832 - 620 pages
...tinis than at others, so that the solar days rnitnot be equal. Another circumstance, dependent upon the inclination of the axis of the earth to the plane of the ecliptic, is nlso to he taken into the account. The apparaît solar time, therefore, is distinguishn 1 from mean...
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Celestial Scenery: Or, The Wonders of the Planetary System Displayed

Thomas Dick - Astronomy - 1838 - 426 pages
...motions and general aspects of the sun in different parts of the earth, which are owing partly to the inclination of the axis of the earth to the plane of the ecliptic, and partly to the different positions in which a spectator is placed in different zones of the globe. It...
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Celestial Scenery: Or, The Wonders of the Planetary System Displayed ...

Thomas Dick - Astronomy - 1838 - 444 pages
...motions and general aspects of the sun in different parts of the earth, which are owing partly to the inclination of the axis of the earth to the plane of the ecliptic, and partly to the different positions in which a spectator is placed in different zones of the globe. It...
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An Outline of a System of Natural Theology

George Crabbe - Natural theology - 1840 - 472 pages
...action from that they manifest singly, and for which there is not a shadow of evidence. The varying inclination of the axis of the earth to the plane of the ecliptic, and the disturbances of the planets by each other's gravity, are rotations, not gradations ; each disturbance...
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Celestial scenery

Thomas Dick - 1840 - 412 pages
...motions and general aspects of the sun in different parts of the earth, which are owing partly to the inclination of the axis of the earth to the plane of the ecliptic, and partly to the different positions in which a spectator is placed in different zones of the globe. It...
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System of universal geography, founded on the works of Malte-Brun and Balbi

System - 1842 - 894 pages
...such, the sphere would appear parallel. As the limits of the zones and of the climates depend upon the inclination of the axis of the earth to the plane of the ecliptic, it is of importance to determine thU inclination. We may easily discover it by observing at the same...
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The popular encyclopedia; or, 'Conversations Lexicon': [ed. by A. Whitelaw ...

Popular encyclopedia - 1846 - 930 pages
...time than at others, so that the solar days cannot be equal. Another circumstance, dependent upon the inclination of the axis of the earth to the plane of the ecliptic, is also to be taken into account. The apparent solar time, therefore, is distinguished from mean solar...
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