Bin 3Af, where the periodical part, which is always to be added to the mean anomaly in order to get the true anomaly, is called the equation of the centre. Spherical Astronomy ... - Pàgina 95per Franz Brünnow - 1865 - 560 pàginesVisualització completa - Sobre aquest llibre
| Franz Brünnow - 1865 - 584 pàgines
...expressed in seconds of arc, we find: v = M-\- 6918" . 37 sin M+ 72" . 52 sin 2 M -h 1" . 05 sin 3M, where the periodical part, which is always to be added...longitude of the sun by adding to v the longitude n which the sun has when the earth is at the perihelion and M -j- n is the longitude of the fictitious... | |
| William Thomas Brande, George William Cox - 1867 - 1090 pàgines
...and mean motion, or the true and mean place of a planet, or the quantity which must be taken from or added to the mean anomaly, in order to get the true anomaly. Let P (or 1") be the place of a planet in its orbit, S the sun, C the centre, and A the perihelion... | |
| Henry Percy Smith - 1883 - 564 pàgines
...and mean motion, or the true and mean place of a planet, or the quantity which must be taken from or added to the mean anomaly in order to get the true anomaly. Prosthesis. (Metaplasm.) Prostyle. [Gr. irpo<rTV\os.] (Arch.) A temple with a row of detached columns... | |
| Henry Percy Smith - 1883 - 542 pàgines
...and mean motion, or the true and mean place of a planet, or the quantity which must be taken from or added to the mean anomaly in order to get the true anomaly. Prosthesis. (Metaplasm.) Prostyle. [Gr. vpoffTv/ios.] (Arch.) A temple with a row of detached columns... | |
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