 | John Frederick William Herschel - 1849 - Страниц: 672
...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 - Страниц: 706
...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 - Страниц: 330
...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 - Страниц: 408
...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 - Страниц: 404
...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 - Страниц: 638
...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 - Страниц: 388
...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 - Страниц: 400
...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 - Страниц: 510
...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 - Страниц: 494
...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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The brightness of objects situated in its nearer portions, therefore, cannot be much exaggerated, nor that of its remoter much enfeebled, by their difference of distance. Yet within this globular space we have collected upwards of... 
