Enviar artigo por via de e-mail Using the К-Means Method for Aggregating the Masses of Elongated Celestial Bodies
- Autores: Burov A.A.1,2, Guerman A.D.3, Nikonov V.I.1,2,3
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Afiliações:
- 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
- Edição: Volume 57, Nº 4 (2019)
- Páginas: 266-271
- Seção: Article
- URL: https://journals.rcsi.science/0010-9525/article/view/153369
- DOI: https://doi.org/10.1134/S0010952519040026
- ID: 153369
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Resumo
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].
Sobre autores
A. Burov
Federal Research Center Informatics and Management, Russian Academy of Sciences; National Research University Higher School of Economics
Email: nikon_v@list.ru
Rússia, Moscow; Moscow
A. Guerman
Centre for Mechanical and Aerospace Science and Technologies, University of Beira Interior
Email: nikon_v@list.ru
Portugal, 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
Autor responsável pela correspondência
Email: nikon_v@list.ru
Rússia, Moscow; Moscow; Covilhã
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