| Ormsby MacKnight Mitchel - 1848 - Liczba stron: 302
...question till he had gone through the second solution. Errors of radius vector were as readily. deducible from the first solution as from the other. The preceding...necessarily be long and laborious. This was the view I took, 82 83 and consequently I had no thought of commencing the search in 1845, the Planet being considerably... | |
| Royal Astronomical Society - 1883 - Liczba stron: 562
...observation, that the mean distance should be still farther diminished. This second solution taken iu conjunction with the first may be considered to relieve...period of great astronomical activity, the planet Astrwa, Biela's double comet, and several other comets, successively demanding attention. During this... | |
| Royal Astronomical Society - 1883 - Liczba stron: 560
...question till he had gone through the second solution. Errors of radius vector were as readily deducible from the first solution as from the other. " The preceding...I had no thought of commencing the search in 1845, tho planet being considerably past opposition at the time Mr. Adams completed his calculations. The... | |
| Walter Libby - 1917 - Liczba stron: 324
...the evidence which the theory gave of the existence of the planet, it might be reasonable to suppose that its position was determined but roughly, and...search for it must necessarily be long and laborious. In the view of Simon Newcomb, 1 Adams's results, which were delivered at the Greenwich Observatory... | |
| 1847 - Liczba stron: 566
...it. No one could have anticipated that the place of the unknown body was indicated with any degree oi exactness by a theory of this kind. It might reasonably...necessarily be long and laborious. This was the view 1 took, and consequently 1 hud no thought of commencing the search in 1845, the planet being considerably... | |
| Liczba stron: 576
...Syndicate1 that it might reasonably be supposed that the position of the planet was only roughly determined, and that a search for it must necessarily be long and laborious. In 1845, when Adams had completed his calculations, the planet was considerably past opposition, and... | |
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