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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... motion Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford University Observatory , Researches in Stellar Parallax by the aid of Photo- graphy , Part 2 , presented by the Observatory ; H. Gyldén , Nouvelles ...
... motion Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford University Observatory , Researches in Stellar Parallax by the aid of Photo- graphy , Part 2 , presented by the Observatory ; H. Gyldén , Nouvelles ...
Page 17
... Motion of the Moon , " part 1 , and I have accepted his graphical interpolation of the individual corrections to the Moon's mean longitude for intervals of a quarter of a century . I then through- out gave each equation of condition the ...
... Motion of the Moon , " part 1 , and I have accepted his graphical interpolation of the individual corrections to the Moon's mean longitude for intervals of a quarter of a century . I then through- out gave each equation of condition the ...
Page 18
... Motion of the Moon . " The terms , however , of dD de δε + d D db Sb . = a became known by substi- tuting the value for de as taken from my table , and for 8b , I took the mean constant value = " 76 as found for it by Professor Newcomb ...
... Motion of the Moon . " The terms , however , of dD de δε + d D db Sb . = a became known by substi- tuting the value for de as taken from my table , and for 8b , I took the mean constant value = " 76 as found for it by Professor Newcomb ...
Page 19
... motions of the perigee and node , in which T represents as before the number of centuries from the epoch 1800 : - and δι ... motion is in a very unsettled state . What is aimed at by astro- nomers is to obtain a constant coefficient ...
... motions of the perigee and node , in which T represents as before the number of centuries from the epoch 1800 : - and δι ... motion is in a very unsettled state . What is aimed at by astro- nomers is to obtain a constant coefficient ...
Page 20
... motion . The facilities for movement in both directions are so great that I have not any doubt that an appa- ratus could be designed that would work well enough to keep the object under examination in the field of view in a sufficiently ...
... motion . The facilities for movement in both directions are so great that I have not any doubt that an appa- ratus could be designed that would work well enough to keep the object under examination in the field of view in a sufficiently ...
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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