 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...  Solutions of the Cambridge Problems: From 1800 to 1820 - Pagina 693door John Martin Frederick Wright - 1825 - 653 pagina’sVolledige weergave - Over dit boek
 | Samuel Vince - 1811 - 260 pagina’s
...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 - 490 pagina’s
...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 - 472 pagina’s
...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 - 876 pagina’s
...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 - 394 pagina’s
...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 - 332 pagina’s
...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 - 304 pagina’s
...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 - 458 pagina’s
...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 - 464 pagina’s
...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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