A modification of gauss' method for preliminary determination of a celestial body's orbit
| dc.contributor.author | Baziei, Oleksandr A. | |
| dc.date.accessioned | 2017-05-18T11:47:48Z | |
| dc.date.available | 2017-05-18T11:47:48Z | |
| dc.date.issued | 2015 | |
| dc.description.abstract | A modification of classical Gauss’ method for determination of Keplerian elements from the observed positions is considered in this paper. The modification involves the exhaustive enumeration of all possible orbital plane positions in order to improve the method’s reliability. It has been shown that such an approach requires a priori information on the pattern of the celestial body's motion, particularly, whether its motion is direct or retrograde. | uk |
| dc.identifier.citation | Odessa Astronomical publications = Одесские астрономические публикации = Одеські астрономічні публікації | uk |
| dc.identifier.uri | https://dspace.onu.edu.ua/handle/123456789/9811 | |
| dc.language.iso | en | uk |
| dc.publisher | Одеський національний університет імені І. І. Мечникова | uk |
| dc.relation.ispartofseries | ;Vol. 28, iss. 2. | |
| dc.subject | orbit determination methods | uk |
| dc.subject | celestial mechanics | uk |
| dc.title | A modification of gauss' method for preliminary determination of a celestial body's orbit | uk |
| dc.type | Article | uk |
Файли
Контейнер файлів
1 - 1 з 1
Ліцензійна угода
1 - 1 з 1
Ескіз недоступний
- Назва:
- license.txt
- Розмір:
- 1.71 KB
- Формат:
- Item-specific license agreed upon to submission
- Опис: