Monthly Notices of the Royal Astronomical SocietyPriestly and Weale, 1861 |
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... equations of condition have shown me that this proposition is true even for the higher powers of the disturbing forces , at least to a considerable extent . I have calculated anew the principal part of the perturba- tions of the ...
... equations of condition have shown me that this proposition is true even for the higher powers of the disturbing forces , at least to a considerable extent . I have calculated anew the principal part of the perturba- tions of the ...
Page 1
... equations - y × 4.63 - 189'0 = 262.1 3 x x × 463 - y x 8.60 by solution of which , x = 93.8 , y = 20 . The rate of change for 1 " , therefore , inferred from the observations , is 20 " , agreeing sensibly with 22 " given by the computed ...
... equations - y × 4.63 - 189'0 = 262.1 3 x x × 463 - y x 8.60 by solution of which , x = 93.8 , y = 20 . The rate of change for 1 " , therefore , inferred from the observations , is 20 " , agreeing sensibly with 22 " given by the computed ...
Page 22
... Equations différentielles rela- tives au Mouvement des Comètes , établies suivant l'hypo- thèse de la force répulsive definie par M. Faye , et suivant l'hypothèse d'un Milieu résistant dans l'espace . Par Jean Plana . ( Turin Memoirs ...
... Equations différentielles rela- tives au Mouvement des Comètes , établies suivant l'hypo- thèse de la force répulsive definie par M. Faye , et suivant l'hypothèse d'un Milieu résistant dans l'espace . Par Jean Plana . ( Turin Memoirs ...
Page 31
... equations of motion are ' = m2 n2 a13 . r I 3 å år ( ) + " - we ♫ ( + { cos 2 p − 2 ) , dt dt 73 2 2 2- -ww-- ) ; m2 n2 d'3 = ( 2 sin 2 v − 2 v ' ) ; = 2 6 -0 ° 10 I -0 ° 2 1Ο -0 ° 02 8 10'1 or writing ... 5 +0 : 03 4 -0.8 d II + 0' ...
... equations of motion are ' = m2 n2 a13 . r I 3 å år ( ) + " - we ♫ ( + { cos 2 p − 2 ) , dt dt 73 2 2 2- -ww-- ) ; m2 n2 d'3 = ( 2 sin 2 v − 2 v ' ) ; = 2 6 -0 ° 10 I -0 ° 2 1Ο -0 ° 02 8 10'1 or writing ... 5 +0 : 03 4 -0.8 d II + 0' ...
Page 43
... equations formed from these data by the method of least squares , I find that the Μας . Ο 4 8 12 84 5 -6 9 99 2 16 Epoch Period = = 1860 , Oct. 17'13 70.88 days Days . 84 20 24 28 32 86 40 44 48 52 00 385 56 60 64 68 70 10.0 Light ...
... equations formed from these data by the method of least squares , I find that the Μας . Ο 4 8 12 84 5 -6 9 99 2 16 Epoch Period = = 1860 , Oct. 17'13 70.88 days Days . 84 20 24 28 32 86 40 44 48 52 00 385 56 60 64 68 70 10.0 Light ...
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2r+g Airy Alhazen Annex appears April Astronomer Royal bright Calculation CAYLEY clock Comet computed corrected crater Decl declination diameter difference distance Ditto ditto edge Ephemeris equations Equatoreal error excentricity eye-piece Greenwich inches aperture instrument July June Jupiter Jupiter's Satellites latitude light limb longitude Lunar m² e m² n² Mars Mean Solar measures Memoir meridian Minor Planets Monthly Notices Moon Moon's Mean Motion N.P.D. from Observation Nautical Almanac nearly Nebula nucleus Number of Observations obtained Occultation orbit parallax perihelion photographs Prof R.A. from Observation Radcliffe Catalogue radiation Right Ascension ring Royal Observatory Saturn Secular Acceleration shadow Sirius Small Planets Society Solar Eclipse soleil stars Struve Sun's disk surface T. W. Webb taches telescope term thermometer tion Transit of Mercury Ursa Variable Variable Stars W. R. Dawes Weisse