 | Samuel Vince - Astronomy - 1811 - 260 pages
...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 - Astronomy - 1816 - 490 pages
...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 - Hydrostatics - 1820 - 472 pages
...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... | |
 | Encyclopedias and dictionaries - 1823 - 876 pages
...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 - Astronomy - 1830 - 394 pages
...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 - Astronomy - 1833 - 324 pages
...negative. 16. Bradley observed, (1). " That each star was farthest north when it came to the meridian about six o'clock in the evening, and farthest south...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 - Circle-squaring - 1846 - 304 pages
...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 - Discoveries in science - 1865 - 460 pages
...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 - Discoveries in science - 1865 - 464 pages
...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... 