Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System
Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System
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In our eReader you can find the full English version of the book. Read Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System
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upon B is f of the attraction upon A, and the disturbing force is i of the attraction upon A.
The disturbmg force in the first case is, therefore.
Digitized by VjOOQIC GREATER THAN AT OPPOSITION. 67 greater than in the second case^in the proportion of 3 to l-, or 27 to 5. This remark applies to nearly all the cases of planet€u>y disturbance where the disturbing planet is exterior to the orbit of the disturbed planet^ the ratio between these distances from the sun being a ratio of not very great... inequality. But it scarcely applies to the moon. For the sun^s distance from the earth is nearly 400 times the moon's distance: conse- quently when the moon is between the sun and the earthy the attraction of the sun on the moon is (i^)* X the attraction of the sun on the earthy OT \tUU par^» of A® sun's attraction on the earthj and the disturbing force therefore is t/AVt parts of the sun'^s attraction on the earth : but when the moon is on that side farthest from the sun^ the sun's attraction on the moon is (iff)* or HHff parts of the sun's attraction on the earthy and the disturbing force is ttWs-t parts of the sun's attraction on the earthy which is very little less than the former.
What to read after Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System?
You can find similar books in the "Read Also" column, or choose other free books by Sir George Biddell Airy to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
upon B is f of the attraction upon A, and the disturbing force is i of the attraction upon A.
The disturbmg force in the first case is, therefore.
Digitized by VjOOQIC GREATER THAN AT OPPOSITION. 67 greater than in the second case^in the proportion of 3 to l-, or 27 to 5. This remark applies to nearly all the cases of planet€u>y disturbance where the disturbing planet is exterior to the orbit of the disturbed planet^ the ratio between these distances from the sun being a ratio of not very great... inequality. But it scarcely applies to the moon. For the sun^s distance from the earth is nearly 400 times the moon's distance: conse- quently when the moon is between the sun and the earthy the attraction of the sun on the moon is (i^)* X the attraction of the sun on the earthy OT \tUU par^» of A® sun's attraction on the earthj and the disturbing force therefore is t/AVt parts of the sun'^s attraction on the earth : but when the moon is on that side farthest from the sun^ the sun's attraction on the moon is (iff)* or HHff parts of the sun's attraction on the earthy and the disturbing force is ttWs-t parts of the sun's attraction on the earthy which is very little less than the former.
What to read after Gravitation; An Elementary Explanation of the Principal Perturbations in the Solar System?
You can find similar books in the "Read Also" column, or choose other free books by Sir George Biddell Airy to read onlineMoreLess
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