I 3 19.4 10 3.8 1 0 29.3 '3 22.3 Ce phenomkne est donc completement analogue P celui qui se produit lors des passages des planetes inferieures sur le disque solaire: et, les observations precedentes montrent que le ligament noir n'est point, pour ainsi dire, une caracteristique de ces passages. On l
Diameters of Mars, at the Opposition of 1881–82
✍ Scribed by C. W. Pritchett
- Publisher
- John Wiley and Sons
- Year
- 1885
- Tongue
- English
- Weight
- 95 KB
- Volume
- 111
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
✦ Synopsis
At the o!iliosition of 1879-80, I measured with the large filar-micrometer of our refractor, a series of groups of the diameters of Mars. These were reduced by Prof. Henry S. Pritchett, (now of Washington University, Saint 1,ouis) and were published in A. N. 2309. At the next opposition, I measured with the same instrument, a much larger series of groups, the whole number of independent measures being 960, or 480 double measures. To publish the whole series of groups, including times, position angles, hour angles, observed diameters and corrections, would require too large a space. I have therefore collected the
📜 SIMILAR VOLUMES
The follon iiig ephemeris is founded upon the same elements as that for tlic preceding opposition, published i n the Monthly Koticcs of the l i . Astronomical Society ~0 1 . 3 9 p.468 f f , the adopted values of the incliiiation and node of the plane of the equator of Mars in rffereiice to that of t
last seen oii Jan. 2 2 , but it was so fai:it :tiid 50 far from the computed poiition that it was :lo: observed. Its estimated paition on this day at 8" m . t . was fi -. I 61'13"'27b d \_: + 2 4 p 24' 8. 0 1 1 accoiint of the very unfavorablz wentiler, thc past winter beii:g the severeit linown in
Saci dem ich durcli I~iuid 3 liiidsay-s ~efldligc JIitLhcilung yon dem neucn Nebcl Kunde erhnltct: Iiatte, ward der Ort merst DEC. 5. (187'3) a m Sucher rnit Hiilftx dci B L>, crniittelt Am G Dcc. Lcobachtete ich den Setwl am (ifuss. Refr. S n 300maliger und an noch starkerer Yergrosserung faiid ich
Observations of Ceres at, the Opposition of 1882. -28.8 -28.7' --. 28.7 -28.3 'The accompanying observations of Ceres were niade by means of the 41/2inch equatorial, those of Sept. 13 with the square bar micrometer, the rest with the filar micrometer. I have corrected the differential measures for
## Mars ' N 12 53 Tauri 6.7 \* -(c) ; hIar8' \* -(C) 8 Nars' N 14 53 Tauri 6.7 \* -(c) 8 Mars' s 15 53 Tauri 6.7 \* -(C) 8 Mars' ?N 16 53 Tauri 6.7 \* -(c) 8 Mars' s 17 53 Tauri 6.7 \* -(c) 8 Mars' N 18 53 Tauri 6.7 \*-(c) 8 Mars' s 19 53 Tauri 6.7 \* -(c) 8, Mars' h 20 53 Tauri 6.7 \* -(c) 8 Mars