On the Connexion of the Physical Sciences |
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Page 10
These two quantities , however , will not give the place of a planet in space . Its distance from the sun ( N. 56 ) must also be known ; and , for the complete determination of its elliptical motion , the nature and position of its ...
These two quantities , however , will not give the place of a planet in space . Its distance from the sun ( N. 56 ) must also be known ; and , for the complete determination of its elliptical motion , the nature and position of its ...
Page 29
Although the apparent diameters of the satellites are too small to be measured , yet their perturbations give the values of their masses with considerable accuracy - a striking proof of the power of analysis .
Although the apparent diameters of the satellites are too small to be measured , yet their perturbations give the values of their masses with considerable accuracy - a striking proof of the power of analysis .
Page 30
... when compared with the time of the eclipse computed for Greenwich , or any other fixed meridian ( N. 95 ) , gives the difference of the meridians in time , and , consequently , the longitude of the place of observation .
... when compared with the time of the eclipse computed for Greenwich , or any other fixed meridian ( N. 95 ) , gives the difference of the meridians in time , and , consequently , the longitude of the place of observation .
Page 43
And , as the lunar theory gives the ratio of the forces , the ratio of the distances of the sun and moon from the earth is obtained . Hence it appears that the sun's mean distance from the earth is 399.7 or nearly 400 times greater than ...
And , as the lunar theory gives the ratio of the forces , the ratio of the distances of the sun and moon from the earth is obtained . Hence it appears that the sun's mean distance from the earth is 399.7 or nearly 400 times greater than ...
Page 43
And , as the lunar theory gives the ratio of the forces , the ratio of the distances of the sun and moon from the earth is obtained . Hence it appears that the sun's mean distance from the earth is 399.7 or nearly 400 times greater than ...
And , as the lunar theory gives the ratio of the forces , the ratio of the distances of the sun and moon from the earth is obtained . Hence it appears that the sun's mean distance from the earth is 399.7 or nearly 400 times greater than ...
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Contents
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Common terms and phrases
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
Bibliographic information
| Title | On the Connexion of the Physical Sciences |
| Author | Mary Somerville |
| Edition | 9 |
| Publisher | J. Murray, 1858 |
| Original from | University of Chicago |
| Digitized | 12 Apr 2012 |
| Length | 523 pages |
| Export Citation | BiBTeX EndNote RefMan |