 | Samuel Vince - 1811 - عدد الصفحات: 260
...Upon comparing the observations with each other, it was discovered, that in both the forementioned stars, the apparent difference of declination from...maxima was always nearly proportional to the versed sir.t of the sun's distance from the equinoctial points. This uas an inducement to think that the cause,... | |
 | John Bonnycastle - 1816 - عدد الصفحات: 490
...comparing the observations with each other, it was discovered, that in both the stars before-mentioned, the apparent difference of declination from the maxima,...of the sun's distance from the equinoctial points. This induced them to think, that the cause, whatever it was, had some relation to the sun's situation... | |
 | Samuel Vince - 1820 - عدد الصفحات: 472
...Upon comparing the observations with each other, it was discovered, that in both the fore-mentioned stars, the apparent difference of declination from...of the sun's distance from the equinoctial points. This was an inducement to think that the cause, whatever it was, had some relation to the sun's situation... | |
 | 1823 - عدد الصفحات: 876
...comparing the observations with each other, it was discovered that, in both the stars above mentioned, the apparent difference of declination from» the...of the sun's distance from the equinoctial points. This was an inducement to think that the cause, whatever it was, had some relation to the sun's situation... | |
 | Miles Bland - 1830 - عدد الصفحات: 394
...to the meridian about six o'clock in the evening, and farthest south when it came about six o'clock in the morning. (2) That in both stars the apparent...apply to stars situated near the solstitial colure. 65. Explain why the effect of aberration on a star not situated in the solstitial colure at 6 o'clock... | |
 | John Martin Frederick Wright - 1833 - عدد الصفحات: 332
...observed, and prove that the horizontal parallax 1 5 X a X cos. dec". " cos. lat. X sin. hour-angle 1 4. If the velocity of the Earth be in a finite ratio...apply to stars situated near the solstitial colure. p . 17- Prove that in elliptical orbits of small eccentricity, the greatest equation to the centre... | |
 | Augustus Young - 1846 - عدد الصفحات: 304
...Upon comparing the observations with each other, it was discovered that in both the fore-mentioned stars, the apparent difference of declination from...of the sun's distance from the equinoctial points. This was an inducement to think that the cause, whatever it was, had some relation to the sun's situation... | |
 | Smithsonian Institution. Board of Regents - 1865 - عدد الصفحات: 458
...Upon comparing tho observations with each other, it was discovered that in both tho before-mentioned stars the apparent difference of declination from the maxima was always nearly proportional to tho versed sine * of the sun's distance from the equinoctial poinU. This was an inducement to think... | |
 | Smithsonian Institution. Board of Regents - 1865 - عدد الصفحات: 464
...discovered that in both tho before-mentioned stars the apparent difference of declination from tho maxima was always nearly proportional to the versed sine* of the sun's distance from tho equinoctial points. This was an inducement to think that the cause, whatever it Tvas, had some... | |
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Upon comparing the observations with each other, it was discovered that in both the fore-mentioned stars, the apparent difference of declination from the maxima was always nearly proportional to the versed sine of the sun's distance from the equinoctial... 