Мақаланы E-mail арқылы жіберу Using the К-Means Method for Aggregating the Masses of Elongated Celestial Bodies
- Авторлар: Burov A.A.1,2, Guerman A.D.3, Nikonov V.I.1,2,3
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Мекемелер:
- Federal Research Center Informatics and Management, Russian Academy of Sciences
- National Research University Higher School of Economics
- Centre for Mechanical and Aerospace Science and Technologies, University of Beira Interior
- Шығарылым: Том 57, № 4 (2019)
- Беттер: 266-271
- Бөлім: Article
- URL: https://journals.rcsi.science/0010-9525/article/view/153369
- DOI: https://doi.org/10.1134/S0010952519040026
- ID: 153369
Дәйексөз келтіру
Ашық рұқсат
Рұқсат берілді
Тек жазылушылар үшін
Аннотация
An approach based on the so-called K-means method has been used to analyze the approximation of gravitational potential of irregularly shaped celestial bodies as the potential of three gravitating balls. Relevant distributions have been constructed for asteroids Bacchus (2063), Kleopatra (216), and Eros (433). The proposed models have been compared with models that are based on alternative approaches [1–3].
Авторлар туралы
A. Burov
Federal Research Center Informatics and Management, Russian Academy of Sciences; National Research University Higher School of Economics
Email: nikon_v@list.ru
Ресей, Moscow; Moscow
A. Guerman
Centre for Mechanical and Aerospace Science and Technologies, University of Beira Interior
Email: nikon_v@list.ru
Португалия, Covilhã
V. Nikonov
Federal Research Center Informatics and Management, Russian Academy of Sciences; National Research University Higher School of Economics; Centre for Mechanical and Aerospace Science and Technologies, University of Beira Interior
Хат алмасуға жауапты Автор.
Email: nikon_v@list.ru
Ресей, Moscow; Moscow; Covilhã
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