The Hill-Brown Theory of the Moons Motion Its Coming-to-be and Short-lived Ascendancy (1877-1984) /
The HillBrown theory of lunar motion was, from its completion in 1908 to its retirement in 1984, the most accurate model of the moons orbit. The mathematical, philosophical, and historical interest in the analytic solution of the lunar problem using the HillBrown method still engages celestial me...
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| Format: | Electronic |
| Language: | English |
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New York, NY :
Springer New York,
2010.
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| Series: | Sources and Studies in the History of Mathematics and Physical Sciences
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| Online Access: | https://ezaccess.library.uitm.edu.my/login?url=http://dx.doi.org/10.1007/978-1-4419-5937-9 |