Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Mariela Huaman"'
Autor:
de Souza, Rafael S., Krone-Martins, Alberto, Carruba, Valerio, Domingos, Rita de Cassia, Ishida, Emille E. O., Alijbaae, Safwan, Espinoza, Mariela Huaman, Barletta, William
Publikováno v:
Res. Notes AAS 5 199 (2021)
The Gaia Data Release 2 provides precise astrometry for nearly 1.5 billion sources across the entire sky, including several thousand asteroids. In this work, we provide evidence that reasonably large asteroids (diameter $>$ 20 km) have high correlati
Externí odkaz:
http://arxiv.org/abs/2108.11814
1. Introduction Linear secular resonances occur when there is a commensurability between the frequency of precession of an asteroid perihelion, g, or node, s, and that of a planet. The ν6 involves a relationship between the frequency g of an asteroi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4dfca73ddeaa8c3d0b25f5d0d10cdc76
https://doi.org/10.5194/epsc2022-238
https://doi.org/10.5194/epsc2022-238
Publikováno v:
Proceedings of the International Astronomical Union. 15:108-112
Close encounters or resonances overlaps can create chaotic motion in small bodies in the Solar System. Approaches that measure the separation rate of trajectories that start infinitesimally near, or changes in the frequency power spectrum of time ser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::587f4ea6291296552e62216d24672e52
https://doi.org/10.1017/s1743921321001307
https://doi.org/10.1017/s1743921321001307
Autor:
Valerio Carruba, Emille E. O. Ishida, Rafael S. de Souza, Mariela Huaman Espinoza, Safwan Alijbaae, William Barletta, R. C. Domingos, Alberto Krone-Martins
Publikováno v:
Res.Notes AAS
Res.Notes AAS, 2021, 5 (8), pp.199. ⟨10.3847/2515-5172/ac205e⟩
Res.Notes AAS, 2021, 5 (8), pp.199. ⟨10.3847/2515-5172/ac205e⟩
The Gaia Data Release 2 provides precise astrometry for nearly 1.5 billion sources across the entire sky, including several thousand asteroids. In this work, we provide evidence that reasonably large asteroids (diameter $>$ 20 km) have high correlati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66d0b65ac5b08cb6a8f27ac36a8eb3fe
https://hal.archives-ouvertes.fr/hal-03327342
https://hal.archives-ouvertes.fr/hal-03327342