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Электронный каталог: Nesterenko, V. V. - Simple Calculation of the Moon Apsides Motion
Nesterenko, V. V. - Simple Calculation of the Moon Apsides Motion
Статья
Автор: Nesterenko, V. V.
Astronomische Nachrichten [Electronic resource]: Simple Calculation of the Moon Apsides Motion
б.г.
ISBN отсутствует
Автор: Nesterenko, V. V.
Astronomische Nachrichten [Electronic resource]: Simple Calculation of the Moon Apsides Motion
б.г.
ISBN отсутствует
Статья
Nesterenko, V.V.
Simple Calculation of the Moon Apsides Motion / V.V.Nesterenko // Astronomische Nachrichten [Electronic resource]. – 2024. – Vol. 345, No. 4. – P. e230143. – URL: https://doi.org/10.1002/asna.20230143. – Bibliogr.: 7.
A simple and clear method to calculate the averaged motion of the apsis linein the Moon orbit is proposed. The obtained result is 3◦1′12′′ for the starryperiod of the Moon revolution around the Earth or 40◦22′48′′ per year. Themodern observed value of the latter quantity is 40◦41′ per year. In “Princip-ia” Newton derived 1◦31′28′′ for the Moon month and 20◦12′′ per year, that isapproximately two times less than the observed values. Contrary to the Newtonapproach, we use a simple and obvious averaging of the Sun disturbing forcefor the starry period of the Moon revolution around the Earth. The applicabilityof the obtained formulae to satellites of other planets and to the planets them-selves is argued. Comparing Newton’s calculation with our method, we revealthe reason, rather convincing, that brought Newton to an imprecise result
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 63 - Астрофизика$
Спец.(статьи,препринты) = С 321 - Классическая механика
Nesterenko, V.V.
Simple Calculation of the Moon Apsides Motion / V.V.Nesterenko // Astronomische Nachrichten [Electronic resource]. – 2024. – Vol. 345, No. 4. – P. e230143. – URL: https://doi.org/10.1002/asna.20230143. – Bibliogr.: 7.
A simple and clear method to calculate the averaged motion of the apsis linein the Moon orbit is proposed. The obtained result is 3◦1′12′′ for the starryperiod of the Moon revolution around the Earth or 40◦22′48′′ per year. Themodern observed value of the latter quantity is 40◦41′ per year. In “Princip-ia” Newton derived 1◦31′28′′ for the Moon month and 20◦12′′ per year, that isapproximately two times less than the observed values. Contrary to the Newtonapproach, we use a simple and obvious averaging of the Sun disturbing forcefor the starry period of the Moon revolution around the Earth. The applicabilityof the obtained formulae to satellites of other planets and to the planets them-selves is argued. Comparing Newton’s calculation with our method, we revealthe reason, rather convincing, that brought Newton to an imprecise result
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 63 - Астрофизика$
Спец.(статьи,препринты) = С 321 - Классическая механика