 | Baden Powell - 1855 - 560 Seiten
...mass, occupying nearly all the space within the earth's orbit — in the haze surrounding more than one of the small planets, and most probably in those...distance from the sun equal to that of the earth, occupied with its nebulosity a sphere greater than that of the whole moon's orbit; and the comet of... | |
 | 1862 - 368 Seiten
...the whole excess in the motion of the perihelion of Mars is attributed to a ring of asteroids situate at a distance from the Sun equal to that of the Earth, the total mass of these asteroids will be somewhat greater than that of Mars, and will be equal to... | |
 | 1862 - 356 Seiten
...the whole excess in the motion of the perihelion of Mars is attributed to a ring of asteroids situate at a distance from the Sun equal to that of the Earth, the total mass of these asteroids will be somewhat greater than that of Mars, and will be equal to... | |
 | Bowdoin College - 1870 - 428 Seiten
...whose hyperbolic trajectory were calculated by if. Petit, director of the observatory of Toulouse. At a distance from the sun equal to that of the earth, a body which owes its motion only to the attraction of the sun, could not have a velocity greater than... | |
 | 1909 - 1064 Seiten
...orbit of the comet for the Earth to meet them at all. There were two positions in which the comet was at a distance from the Sun equal to that of the Earth : on one side the distance from the Earth's orbit was 6 million miles, and on the other side it was... | |
 | 1917 - 498 Seiten
...— which is usually called the temperature of space. It is not difficult to see how this happens. At a distance from the Sun equal to that of the Earth a black body would take up a temperature of 280° absolute. Now suppose we have a body which can absorb... | |
 | John Henry Poynting - 1920 - 810 Seiten
...receive radiation from the sun. Temperature of a Planet under Certain Assumed Conditions when placed at a Distance from the Sun equal to that of the Earth. The real earth presents a problem of complexity far too great to deal with. I shall therefore consider... | |
 | 1917 - 892 Seiten
...sufficient to fix clearly the order of magnitude of the phenomena. First let us place the testing body at a distance from the sun equal to that of the earth. The radiating body then has an apparent diameter of 32' and we find In M= 12.1. Taking c= 14,350 micron-degrees,... | |
 | 1954 - 814 Seiten
...receive radiation from the sun. Temperature of a Planet under Certain Assumed Conditions wJien placed at a Distance from the Sun equal to that of the Earth. The real earth presents a problem of complexity far too great to deal with. I shall therefore consider... | |
 | 1917 - 530 Seiten
...— which is usually called the temperature of space. It is not diliicult to see how this happens. At a distance from the Sun equal to that of the Earth a black body would take up a temperature of 280° absolute. Now suppose we have a body which can absorb... | |
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... or about 125 watts/foot . Most of this energy is in the visible portion of the spectrum. The intensity of this solar flux in other portions of the solar system... 