Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Włodarczyk Ireneusz"'
Autor:
Włodarczyk Ireneusz, Černis Kazimieras
Publikováno v:
Open Astronomy, Vol 31, Iss 1, Pp 244-255 (2022)
This article is devoted to the discovery of comets at the Vilnius Observatory together with the orbital analysis of dynamically interesting comets, namely 322P. We studied the orbital evolution of comet 322P with and without non-gravitational effects
Externí odkaz:
https://doaj.org/article/bc1fcedca7864c98aad3ed6850412bb0
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 35-47 (2017)
This paper is devoted to the discovery of asteroids at the Molėtai Astronomical Observatory (MAO) in 2010- 2012 together with the orbital analysis of two dynamically interesting Near Earth Objects (NEOs) discovered at the MAO, namely 2006 SF77 and 2
Externí odkaz:
https://doaj.org/article/fcdd3e42c4004cb2b42ca4c28c656e40
Publikováno v:
A&A 646, A182 (2021)
Dynamical studies of asteroid populations in retrograde orbits, that is with orbital inclinations greater than 90 degrees, are interesting because the origin of such orbits is still unexplained. Generally, the population of retrograde asteroids inclu
Externí odkaz:
http://arxiv.org/abs/2101.04364
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
The population of known minor bodies in retrograde orbits ($i > 90 ^{\circ}$) that are classified as asteroids is still growing. The aim of our study was to estimate the dynamical lifetimes of these bodies by use of the latest observational data, inc
Externí odkaz:
http://arxiv.org/abs/1703.01824
Publikováno v:
A&A 584, A18 (2015)
Most asteroid families are very homogeneous in physical properties. Some show greater diversity, however. The Flora family is the most intriguing of them. The Flora family is spread widely in the inner main belt, has a rich collisional history, and i
Externí odkaz:
http://arxiv.org/abs/1510.00865
Autor:
Kankiewicz, Paweł a, ∗, Włodarczyk, Ireneusz b
Publikováno v:
In Planetary and Space Science May 2018 154:72-76
Publikováno v:
Astron.Astrophys. 405 (2003) 1145-1152
Mean motion resonances (MMRs) can lead either to chaotic or regular motion. We report on a numerical experiment showing that even in one of the most chaotic regions of the Solar System - the region of the giant planets, there are numerous bands where
Externí odkaz:
http://arxiv.org/abs/astro-ph/0203182
Publikováno v:
In Planetary and Space Science January 2012 60(1):181-192