Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Kirkwood gap"'
Many asteroids in the main belt are continuously pushed by Yarkovsky effect into regions of different mean motion resonances (MMRs) and then ejected out. They are considered as the principal source of near-Earth objects. We investigate in this paper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c8ffa87975dd6c9a8370fa8bd99f257
http://arxiv.org/abs/2002.08794
http://arxiv.org/abs/2002.08794
Autor:
S. K. Fieber-Beyer, Michael J. Gaffey
Publikováno v:
Icarus. 257:113-125
The research is an integrated effort beginning with telescopic observations and extending through detailed mineralogical characterizations to provide constraints on the composition and meteorite affinities of a subset of fourteen asteroids in/near th
Autor:
S. K. Fieber-Beyer, Michael J. Gaffey
Publikováno v:
Icarus. 229:99-108
The 3:1 Kirkwood Gap asteroids are a mineralogically diverse set of asteroids located in a region that delivers meteoroids into Earth-crossing orbits. Mineralogical characterizations of asteroids in/near the 3:1 Kirkwood Gap can be used as a tool to
Publikováno v:
Icarus. 221:593-602
The 3:1 Kirkwood gap asteroids are a mineralogically diverse set of asteroids located in a region that delivers meteoroids into Earth-crossing orbits. Mineralogical characterizations of asteroids in/near the 3:1 Kirkwood Gap can be used as a tool to
Autor:
Chalbeth M. Reynolds, Vishnu Reddy, Michael J. Gaffey, M. S. Kelley, Tony Hicks, S. K. Fieber-Beyer
Publikováno v:
Icarus. 213:524-537
We present a mineralogical assessment of 12 Maria family asteroids, using near-infrared spectral data obtained over the years 2000–2009 combined with visible spectral data (when available) to cover the spectral interval of 0.4–2.5 μm. Our analys
Short-lived asteroids in the 7/3 Kirkwood gap and their relationship to the Koronis and Eos families
Publikováno v:
Icarus. 166:131-140
A population of 23 asteroids is currently observed in a very unstable region of the main belt, the 7 /3 Kirkwood gap. The small size of these bodies—with the notable exception of (677) Aaltje (∼ 30 km)—as well as the computation of their dynami
Autor:
Guillermo González-Casado, Miquel Grau
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 72:169-186
A comparative study of the evolution of the Sun–Jupiter–Asteroid system near the 4:1 and 7:2 resonances is performed by means of two techniques that proceed differently from the Hamiltonian corresponding to the planar restricted elliptic three-bo
Autor:
Nishimura, Hitoshi, Yoshikawa, Makoto
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :143-145
資料番号: AA0063350039
Publikováno v:
Planetary and Space Science. 45:1581-1585
After discovering that asteroid (2953) Vysheslavia, a Koronis family member, has a typical dynamical lifetime of the order of 10 Myr only against “falling” into the 5:2 Kirkwood gap and ending up in a hyperbolic orbit (Milani and Farinella, 1995.
Autor:
Jan Vrbik
Publikováno v:
Journal of Physics A: Mathematical and General. 29:3311-3316
A mathematical description of the Kirkwood gap in the 2/1 resonance with Jupiter is discussed in detail, providing a new insight into a traditionally controversial issue. The discussion is further extended to demonstrate how, under slightly different