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 37
... orbit . At present the 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 ...
... orbit . At present the 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 ...
Page 41
... orbital movement of C about the close pair , can , of course , be wholly neglected , since that will be a constant quantity . In the interest of the solution of this question I have put these suggestions in practice , and have made each ...
... orbital movement of C about the close pair , can , of course , be wholly neglected , since that will be a constant quantity . In the interest of the solution of this question I have put these suggestions in practice , and have made each ...
Page 44
... Orbit of Σ 2525. By J. E. Gore . A recent measure of this binary star made by Mr. Burnham with the 36 - inch refractor of the Lick Observatory shows that the companion has described about 288 ° of its apparent ellipse since its ...
... Orbit of Σ 2525. By J. E. Gore . A recent measure of this binary star made by Mr. Burnham with the 36 - inch refractor of the Lick Observatory shows that the companion has described about 288 ° of its apparent ellipse since its ...
Page 45
... Orbit of y Corona Australis . By R. P. Sellors , B.A. ( Communicated by H. C. Russell , B.A. , F.R.S. ) The general equation of the apparent ellipse was found by Glasenapp's method , and the geometrical elements deduced therefrom by the ...
... Orbit of y Corona Australis . By R. P. Sellors , B.A. ( Communicated by H. C. Russell , B.A. , F.R.S. ) The general equation of the apparent ellipse was found by Glasenapp's method , and the geometrical elements deduced therefrom by the ...
Page 46
... I'32 1'47 -'15 I -13 83.620 Wilson 217.7 2170 + 0'7 86.615 Pollock 3 142 1.46 4 165 146 -'04 2 + '20 I 2006 2015-09 8 145 145 '00 8 Epoch . No. of Observer . θα eco Nights . 46 LIII . I , Mr. Sellors , The Orbit of.
... I'32 1'47 -'15 I -13 83.620 Wilson 217.7 2170 + 0'7 86.615 Pollock 3 142 1.46 4 165 146 -'04 2 + '20 I 2006 2015-09 8 145 145 '00 8 Epoch . No. of Observer . θα eco Nights . 46 LIII . I , Mr. Sellors , The Orbit of.
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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