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 36
... Satellite of Jupiter . By E. E. Barnard , M.A. This satellite was discovered here by the writer at midnight , 1892 , September 9 , with the 36 - inch equatoreal . From the eastern elongations of September 10 and October 21 the following ...
... Satellite of Jupiter . By E. E. Barnard , M.A. This satellite was discovered here by the writer at midnight , 1892 , September 9 , with the 36 - inch equatoreal . From the eastern elongations of September 10 and October 21 the following ...
Page 37
... satellite is assumed to be of the 13th magnitude . Under the most favourable conditions it has not been possible to see the shadow of this object when in transit . From these and other considerations the satellite is probably not over ...
... satellite is assumed to be of the 13th magnitude . Under the most favourable conditions it has not been possible to see the shadow of this object when in transit . From these and other considerations the satellite is probably not over ...
Page 38
Royal Astronomical Society. I prefer to compare the motion of the new satellite with that of the first hitherto known satellite of Jupiter . The exact formula to be employed is P == M + m , R3 PM + mR where M is the mass of Jupiter , mo ...
Royal Astronomical Society. I prefer to compare the motion of the new satellite with that of the first hitherto known satellite of Jupiter . The exact formula to be employed is P == M + m , R3 PM + mR where M is the mass of Jupiter , mo ...
Page 39
... satellite between the times of two distant elongations , as has now been done by Mr. A. Marth and Professor Barnard , whose periods thereby derived agree within half a second of time . The period found by Mr. Marth is 11h 57m.33 . 1892 ...
... satellite between the times of two distant elongations , as has now been done by Mr. A. Marth and Professor Barnard , whose periods thereby derived agree within half a second of time . The period found by Mr. Marth is 11h 57m.33 . 1892 ...
Page 135
... They are also corrected for the error of inclination of the wires , and , where necessary , for the motion of the comet in N.P.D. Phenomena of Jupiter's Satellites . Day . Satellite . Phenomenon Jan. 1893 . 135 of Brooks ' Comet .
... They are also corrected for the error of inclination of the wires , and , where necessary , for the motion of the comet in N.P.D. Phenomena of Jupiter's Satellites . Day . Satellite . Phenomenon Jan. 1893 . 135 of Brooks ' Comet .
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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