电邮这篇文章 Using the К-Means Method for Aggregating the Masses of Elongated Celestial Bodies
- 作者: Burov A.A.1,2, Guerman A.D.3, Nikonov V.I.1,2,3
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隶属关系:
- 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
- 期: 卷 57, 编号 4 (2019)
- 页面: 266-271
- 栏目: Article
- URL: https://journals.rcsi.science/0010-9525/article/view/153369
- DOI: https://doi.org/10.1134/S0010952519040026
- ID: 153369
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详细
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].
作者简介
A. Burov
Federal Research Center Informatics and Management, Russian Academy of Sciences; National Research University Higher School of Economics
Email: nikon_v@list.ru
俄罗斯联邦, Moscow; Moscow
A. Guerman
Centre for Mechanical and Aerospace Science and Technologies, University of Beira Interior
Email: nikon_v@list.ru
葡萄牙, 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
编辑信件的主要联系方式.
Email: nikon_v@list.ru
俄罗斯联邦, Moscow; Moscow; Covilhã
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