On possible planetary close approaches to high inclination asteroids
The orbital evolution of fictitious high inclination main belt asteroids with movement corresponding to the conditions of the Tisserand invariant for C =C(L1) in the restricted three-body problem has been investigated. The obtained results showed that the bodies with inclinations within 40–80° and 1...
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National Aviation University
2004-12-01
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| Series: | Вісник Астрономічної школи |
| Online Access: | http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/016.html |
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doaj-feda76e4fe5a4dc7bcc5eefefc8aeb1e2020-11-25T03:22:03ZengNational Aviation UniversityВісник Астрономічної школи1607-28552411-66022004-12-0151-2162210.18372/2411-6602.05.10162411-6602.05.1016On possible planetary close approaches to high inclination asteroidsN. A. Solovaya0E. M. Pittikh1Astronomical Institute of Slovak Academy of Sciences, Slovak RepublicAstronomical Institute of Slovak Academy of Sciences, Slovak RepublicThe orbital evolution of fictitious high inclination main belt asteroids with movement corresponding to the conditions of the Tisserand invariant for C =C(L1) in the restricted three-body problem has been investigated. The obtained results showed that the bodies with inclinations within 40–80° and 100–140° and eccentricities within 0.0–0.4 are dynamically stable at least during the 200 000 years investigated period, and periodically change their inclinations, eccentricities and perihelion distances. In some time, they can reach the vicinity of the Sun and during their orbital evolution they cross orbits of the inner planets many times.http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/016.html |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
N. A. Solovaya E. M. Pittikh |
| spellingShingle |
N. A. Solovaya E. M. Pittikh On possible planetary close approaches to high inclination asteroids Вісник Астрономічної школи |
| author_facet |
N. A. Solovaya E. M. Pittikh |
| author_sort |
N. A. Solovaya |
| title |
On possible planetary close approaches to high inclination asteroids |
| title_short |
On possible planetary close approaches to high inclination asteroids |
| title_full |
On possible planetary close approaches to high inclination asteroids |
| title_fullStr |
On possible planetary close approaches to high inclination asteroids |
| title_full_unstemmed |
On possible planetary close approaches to high inclination asteroids |
| title_sort |
on possible planetary close approaches to high inclination asteroids |
| publisher |
National Aviation University |
| series |
Вісник Астрономічної школи |
| issn |
1607-2855 2411-6602 |
| publishDate |
2004-12-01 |
| description |
The orbital evolution of fictitious high inclination main belt asteroids with movement corresponding to the conditions of the Tisserand invariant for C =C(L1) in the restricted three-body problem has been investigated. The obtained results showed that the bodies with inclinations within 40–80° and 100–140° and eccentricities within 0.0–0.4 are dynamically stable at least during the 200 000 years investigated period, and periodically change their inclinations, eccentricities and perihelion distances. In some time, they can reach the vicinity of the Sun and during their orbital evolution they cross orbits of the inner planets many times. |
| url |
http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/016.html |
| work_keys_str_mv |
AT nasolovaya onpossibleplanetarycloseapproachestohighinclinationasteroids AT empittikh onpossibleplanetarycloseapproachestohighinclinationasteroids |
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1724611468591104000 |