Monthly Notices of the Royal Astronomical Society, Volume 68; Volumes 1907-1908Priestley and Weale, 1908 Includes lists of additions to the Society's library, usually separately paged. |
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Page 33
... computed from the data given in the Con- naissance des Temps , based on Dr. Hermann Struve's elements , the eccentricity of the orbit being neglected . A discussion of these residuals gives the following differences from Dr. Hermann ...
... computed from the data given in the Con- naissance des Temps , based on Dr. Hermann Struve's elements , the eccentricity of the orbit being neglected . A discussion of these residuals gives the following differences from Dr. Hermann ...
Page 123
... computed the perturbations by Jupiter and Saturn only for the revolutions 1531 to 1607 , 1607 to 1682 , his value is obviously not to be relied on beyond the first decimal . Revolution 1378 to 1456 . Planet . Limits of u . Sdn . A. O O ...
... computed the perturbations by Jupiter and Saturn only for the revolutions 1531 to 1607 , 1607 to 1682 , his value is obviously not to be relied on beyond the first decimal . Revolution 1378 to 1456 . Planet . Limits of u . Sdn . A. O O ...
Page 148
... computation of the terms in the Moon's motion due to the actions - direct and indirect - of the planets , and it is of interest to compare the results with those of previous investigators . There are two extensive lists in print : one ...
... computation of the terms in the Moon's motion due to the actions - direct and indirect - of the planets , and it is of interest to compare the results with those of previous investigators . There are two extensive lists in print : one ...
Page 149
... computed to o " oor except those of a few long period terms in dw1 ; these exceptions are noted by a comma placed before the zero , which is set down as the last figure in order not to break the continuity of the representation . 7 , 2D ...
... computed to o " oor except those of a few long period terms in dw1 ; these exceptions are noted by a comma placed before the zero , which is set down as the last figure in order not to break the continuity of the representation . 7 , 2D ...
Page 167
... computation of de unnecessary except in a few easily recognised cases . 6. One other fact should be noted . Although the coefficient of the evection ( arg . 2D ) is of order m ( 1/13 ) compared with that of the principal elliptic term ...
... computation of de unnecessary except in a few easily recognised cases . 6. One other fact should be noted . Although the coefficient of the evection ( arg . 2D ) is of order m ( 1/13 ) compared with that of the principal elliptic term ...
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Common terms and phrases
angle appear Astrographic axis bright brighter Cape Catalogue centre coefficient colour column comet comparison stars computed corrections correlation curve cyanogen David Gill deduced determination distance Double Stars drift E. E. Barnard Earth eclipse epoch equation equatorial faint formula give given Greenwich groups heliometer instrument Julian Day Jupiter latitude lens Lick Observatory limb lines longitude magnitude Max Wolf mean measures meridian method Monthly Notices Moon nebula nucleus number of stars observations obtained orbit outer condensation paper parallax Paris perihelion perihelion passage period perturbations photographs planet plates position present Professor proper motion reduced reflector refraction refractor region right ascension ring Royal Observatory satellite Saturn seen Sept solar spectra spectral class spectroheliograph spectroscope spectrum spot stellar sun-spot Sun's surface Table telescope tion variable Yerkes Observatory zone ΙΟ