| John Frederick William Herschel - 1849 - 672 páginas
...stars as compared one with another. Taking the apparent semidiameter of the nubecula major at 3°, and regarding its solid form as, roughly speaking,...than a tenth part of our distance from its centre. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor... | |
| John Frederick William Herschel - 1851 - 704 páginas
...stars as compared one with another. Taking the apparent semidiameter of the nubecula major at 3°, and regarding its solid form as, roughly speaking,...little more than a tenth part of our distance from its center. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated,... | |
| William Whewell - 1854 - 330 páginas
...nearest and most remote parts must (as its angular size proves) differ in their distance from us by little more than a tenth part of our distance from its centre. That the two nubeculae are thus approximately spherical spaces, is in the highest degree probable ;... | |
| 1855 - 408 páginas
...any other region of the heavens." ' Taking the apparent semidiameter of the Nubecula Major at 3 °, and regarding its solid form as, roughly speaking,...than a tenth part of our distance from its centre. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor... | |
| William Whewell - 1855 - 404 páginas
...nearest and most remote parts must (as its angular size proves) differ in their distance from us by little more than a tenth part of our distance from its centre. That the two nubeculee are thus approximately spherical spaces, is in the highest degree probable ;... | |
| John Holmes Agnew, Walter Hilliard Bidwell, Henry T. Steele - 1858 - 638 páginas
...compared with one another. Taking the apparent semi-diameter of the nubécula major at three degrees, and regarding its solid form as, roughly speaking,...little more than a tenth part of our distance from its center. The brightness of objects situated in its nearer 1858.] portions, therefore, can not be much... | |
| Herbert Spencer - 1864 - 400 páginas
...compared with one another. Taking the apparent semi-diameter of the nubecula major at three degrees, and regarding its solid form as, roughly speaking,...than a tenth part of our distance from its centre. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor... | |
| Herbert Spencer - 1864 - 388 páginas
...compared with one another. Taking the apparent semi-diameter of the nubecula major at three degrees, and regarding its solid form as, roughly speaking,...than a tenth part of our distance from its centre. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor... | |
| Herbert Spencer - 1864 - 510 páginas
...compared with one another. Taking the apparent semi-diameter of the nnbecula major at three degrees, and regarding its solid form as, roughly speaking,...differ in their distance from us by a little more tlian a tenth part of our distance from its centre. The brightness of objects situated in its nearer... | |
| Herbert Spencer - 1867 - 494 páginas
...compared with one another. Taking the apparent semi-diameter of the nubecula mnjor at three degrees, ami regarding its solid form as, roughly speaking, spherical,...than a tenth part of our distance from its centre. The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor... | |
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