 | Sir John Frederick William Herschel - 1833 - 444 lapas
...analogous to our [trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it...disc, but fade away gradually before they reach it. (See Plate I. fig. 2.) The apparent diameter of Jupiter varies from 30" to 46". (441.) A still more... | |
 | sir John Frederick W. Herschel (1st bart.) - 1833 - 500 lapas
...analogous to our [trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it...disc, but fade away gradually before they reach it. (See Plate I. fig. 2.) The apparent diameter of Jupiter varies from 30" to 46". (441.) A still more... | |
 | 1835 - 480 lapas
...analogous to our trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it is the comparatively dark body of the planet which appears in the belts, is evident from this — that they do not come... | |
 | Thomas Dick - 1838 - 426 lapas
...body at a considerable elevation, it has been observed by Sir John Herschel, " that the dark belts do not come up in all their strength to the edge of the disk, but fade away gradually before they reach it ;" an almost decisive proof that the bright belts... | |
 | Thomas Dick - 1838 - 444 lapas
...body at a considerable elevation, it has been observed by Sir John Herschel, " that the dark belts do not come up in all their strength to the edge of the disk, but fade away gradually before they resch it ;" an almost decisive proof that the bright belts... | |
 | John Frederick William Herschel - 1849 - 672 lapas
...analogous to our trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it...planet which appears in the belts is evident from this,—that they do not come up in all their strength to the edge of the disc, but fade away gradually... | |
 | Thomas Dick - 1850 - 586 lapas
...body at a considerable elevation, it has been observed by Sir John Herschcl, " that the dark belts do not come up in all their strength to the edge of the disk, but fado away gradually before they reach it;" an almost decisive proof that the bright belts... | |
 | John Frederick William Herschel - 1851 - 744 lapas
...analogous to our trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it...disc, but fade away gradually before they reach it. ( See Plate HI. Jig. 2.) The apparent diameter of Jupiter varies from 30" to 46". (514.) A still more... | |
 | William Augustus Norton - 1852 - 522 lapas
...necessary consequence of tin- superior velocity of rotation of this planet. As remarked by Herschel, that it is the comparatively darker body of the planet...disc, but fade away gradually before they reach it The bright belts, intermediate between the dark ones, are probably baud* of clouds or tracts of less... | |
 | John Frederick William Herschel - 1853 - 608 lapas
...analogous to our trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it...their strength to the edge of the disc, but fade away gtadually before they reach it. (See Plate III. fig, 2.) The apparent diameter of Jupiter varies from... | |
| |
... appearances of spots seen upon them, render it extremely probable that they subsist in the atmosphere of the planet, forming tracts of comparatively clear sky, determined by currents analogous to our trade-winds, but of a much more steady and decided... 
