The Hill-Brown Theory of the Moon’s Motion Its Coming-to-be and Short-lived Ascendancy (1877-1984) /
The Hill–Brown theory of lunar motion was, from its completion in 1908 to its retirement in 1984, the most accurate model of the moon’s orbit. The mathematical, philosophical, and historical interest in the analytic solution of the lunar problem using the Hill–Brown method still engages celestial me...
| Κύριος συγγραφέας: | |
|---|---|
| Συγγραφή απο Οργανισμό/Αρχή: | |
| Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
| Γλώσσα: | English |
| Έκδοση: |
New York, NY :
Springer New York,
2010.
|
| Σειρά: | Sources and Studies in the History of Mathematics and Physical Sciences
|
| Θέματα: | |
| Διαθέσιμο Online: | Full Text via HEAL-Link |
