Monthly Notices of the Royal Astronomical Society, Volume 53; Volumes 1892-1893Priestley and Weale, 1893 Includes lists of additions to the Society's library, usually separately paged. |
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Page 13
... method is the number of gaps in the different series ; and as a first attempt two or three years were taken together to remedy this defect . The resulting predictions for January and February 1893 were com- pared Nov. 1892 . 13 Moon in ...
... method is the number of gaps in the different series ; and as a first attempt two or three years were taken together to remedy this defect . The resulting predictions for January and February 1893 were com- pared Nov. 1892 . 13 Moon in ...
Page 14
... method in a case of this kind . From what has been said above , it will be clear that this note is in no way intended as a serious contribution to lunar theory . It will be seen that predictions were not made for the earlier days in ...
... method in a case of this kind . From what has been said above , it will be clear that this note is in no way intended as a serious contribution to lunar theory . It will be seen that predictions were not made for the earlier days in ...
Page 22
... method . A reason for this neglect of the probable error of the clock rate may be the difficulty of determining it when another quite common practice is followed of determining the clock rate from the comparison of the clock corrections ...
... method . A reason for this neglect of the probable error of the clock rate may be the difficulty of determining it when another quite common practice is followed of determining the clock rate from the comparison of the clock corrections ...
Page 44
... method , and find the following provisional elements : - Elements of 2525 . P = 138.54 years . T = 1887.12 e = 0.802 i = 54 ° o ' 8 = 78 ° 19'5 λ = 4 ° 19 ' a = 0 " +75 μ = -2 ° .5984 The following is a comparison between the measures ...
... method , and find the following provisional elements : - Elements of 2525 . P = 138.54 years . T = 1887.12 e = 0.802 i = 54 ° o ' 8 = 78 ° 19'5 λ = 4 ° 19 ' a = 0 " +75 μ = -2 ° .5984 The following is a comparison between the measures ...
Page 45
... method , and the geometrical elements deduced therefrom by the formula of Kowalsky . The dynamical ele- ments were determined from five equations of mean motion . P = 12124 years T = 1879'33 e = 0 * 33096 i = 35 ° 37 Elements . 8 = 57 ...
... method , and the geometrical elements deduced therefrom by the formula of Kowalsky . The dynamical ele- ments were determined from five equations of mean motion . P = 12124 years T = 1879'33 e = 0 * 33096 i = 35 ° 37 Elements . 8 = 57 ...
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Common terms and phrases
Academy Andromedæ angle appeared Aquilæ Astronomer Royal Auriga Bisection bright Burnham Camelop Canis Carinæ Cassiopeia Catalogue Centauri centre Cephei cluster coefficient comet comparison stars correction Cygni Dembowski determined diameter distance double stars E. E. Barnard eclipse epoch Equat equatoreal exposure Galactic Long Geminorum Greenwich Greenwich Mean instrument Isaac Roberts June Jupiter Lalande lens Lick Observatory London longitude lunar Lupi Magn magnitude me²e mean measures Meteorological micrometer Monocerotis Monthly Notices Moon motion nebula Nova Auriga observations obtained Ophiuchi orbit Orionis paper parallax Paris period Persei photographs planet plates position probable error Professor proper motion Puppis Refraction right ascension Royal Observatory S. W. Burnham Sagittarii satellite Saturn Schiaparelli Scorpii seen Sept solar spectra spectroscope spectrum stellar Struve Tauri telescope thermometer tion transit transit circle Velorum ΙΟ