Monthly Notices of the Royal Astronomical Society, Volume 53Priestley and Weale, 1893 Includes lists of additions to the society's library, usually separately paged. |
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Page 17
... equation of condition the weight of unity , as I look with suspicion on assigning different weights to the observations . I took out from the theory all of Hansen's terms of long period due to the action of the planets on the Moon , and ...
... equation of condition the weight of unity , as I look with suspicion on assigning different weights to the observations . I took out from the theory all of Hansen's terms of long period due to the action of the planets on the Moon , and ...
Page 24
... equation ( 2 ) . The probable error of the clock correction at any moment will then be found by ( 1 ) or ( 3 ) . 00 Since the squares of the probable errors of the quantities found by a least squares solution are inversely proportional ...
... equation ( 2 ) . The probable error of the clock correction at any moment will then be found by ( 1 ) or ( 3 ) . 00 Since the squares of the probable errors of the quantities found by a least squares solution are inversely proportional ...
Page 26
... equation in p by that in its own normal equation . It will , in general , differ from [ wde ] [ wee ] the mean of the times of observation . = - In the example given below the square brackets are used also to indicate the number whose ...
... equation in p by that in its own normal equation . It will , in general , differ from [ wde ] [ wee ] the mean of the times of observation . = - In the example given below the square brackets are used also to indicate the number whose ...
Page 45
... equation of the apparent ellipse was found by Glasenapp's method , and the geometrical elements deduced therefrom by the formula of Kowalsky . The dynamical ele- ments were determined from five equations of mean motion . P = 12124 years ...
... equation of the apparent ellipse was found by Glasenapp's method , and the geometrical elements deduced therefrom by the formula of Kowalsky . The dynamical ele- ments were determined from five equations of mean motion . P = 12124 years ...
Page 117
... equation di Р = dt Also ( yZ - zY ) sin & cos i + ( xZ - zX ) cos & cos i- ( xY - yX ) sin i . P sin i d8 dt 4 = ( yZ — ≈Y ) cos 2 − ( xZ − zX ) sin 8 . ---- Hitherto we have left the positions of the rectangular coor- dinate axes ...
... equation di Р = dt Also ( yZ - zY ) sin & cos i + ( xZ - zX ) cos & cos i- ( xY - yX ) sin i . P sin i d8 dt 4 = ( yZ — ≈Y ) cos 2 − ( xZ − zX ) sin 8 . ---- Hitherto we have left the positions of the rectangular coor- dinate axes ...
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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