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 17
... distance of the Moon from the plane of the Sun's equator , when the Moon arrives at conjunction with the Sun. The following is the correction to the Moon's mean longitude which I have determined : - : - In which de = dv + dnz . And dv + ...
... distance of the Moon from the plane of the Sun's equator , when the Moon arrives at conjunction with the Sun. The following is the correction to the Moon's mean longitude which I have determined : - : - In which de = dv + dnz . And dv + ...
Page 29
... distance from the centre would appreciably affect the determination of photographic magnitude . The following are the values of photographic magnitude of BD + 30 ° 898 deduced in the two cases : - Star 60 ' from centre of plate ...
... distance from the centre would appreciably affect the determination of photographic magnitude . The following are the values of photographic magnitude of BD + 30 ° 898 deduced in the two cases : - Star 60 ' from centre of plate ...
Page 35
... distance A E seems to be increasing . If this is real , and it seems to be so , it is strange that before my observations , it is not apparent , as compared with those of Mr. Burnham . Measures will be made to decide whether this motion ...
... distance A E seems to be increasing . If this is real , and it seems to be so , it is strange that before my observations , it is not apparent , as compared with those of Mr. Burnham . Measures will be made to decide whether this motion ...
Page 36
... distance of the satellite ( at east elongation ) is 48 " 094 ( at 5.20 ) . This corre- sponds to a distance from Jupiter's centre of 112,510 miles . The few observed western elongations give a distance about I " less than this , and ...
... distance of the satellite ( at east elongation ) is 48 " 094 ( at 5.20 ) . This corre- sponds to a distance from Jupiter's centre of 112,510 miles . The few observed western elongations give a distance about I " less than this , and ...
Page 37
... distance at east elongation of the 23rd was- October 26 . 62 " 90 On the Sidereal Period of the New Satellite of ... distances of the satellite at its elongations , September 10 , 12 , and 14 . Professor Barnard employs the formula— P ...
... distance at east elongation of the 23rd was- October 26 . 62 " 90 On the Sidereal Period of the New Satellite of ... distances of the satellite at its elongations , September 10 , 12 , and 14 . Professor Barnard employs the formula— P ...
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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