Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Proper orbital elements"'
Publikováno v:
Astronomy & Astrophysics. 649:A115
Very young asteroid families may record processes that accompanied their formation in the most pristine way. This makes analysis of this special class particularly interesting. We studied the very young Adelaide family in the inner part of the main b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2884832fe3a605152db27e59e84d66ba
https://doi.org/10.1051/0004-6361/202140421
https://doi.org/10.1051/0004-6361/202140421
Autor:
Vania Lorenzi, Humberto Campins, Zoe A. Landsman, Javier Licandro, Marco Delbo, V. Alí-Lagoa, Michael P. Lucas, Brian Burt, Francesca E. DeMeo, Kevin J. Walsh, J. de León, Noemi Pinilla-Alonso
Publikováno v:
Icarus. 274:231-248
The inner asteroid belt is an important source of near-Earth asteroids (NEAs). Dynamical studies of the inner asteroid belt have identified several families overlapping in proper orbital elements, including the Polana and Eulalia families that contai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1a33016f8776bcf37fb72fdda1555d5
https://doi.org/10.1016/j.icarus.2016.03.022
https://doi.org/10.1016/j.icarus.2016.03.022
Publikováno v:
Icarus. 243:111-128
The Flora family resides in the densely populated inner main belt, bounded in semimajor axis by the $\nu_6$ secular resonance and the Jupiter 3:1 mean motion resonance. The presence of several large families that overlap dynamically with the Floras (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7287a9b9d8b42f3d82d0c8e1ab3bc68b
https://doi.org/10.1016/j.icarus.2014.09.011
https://doi.org/10.1016/j.icarus.2014.09.011
Publikováno v:
Icarus. 162:308-327
Asteroid families are groupings of minor planets identified by clustering in their proper orbital elements; these objects have spectral signatures consistent with an origin in the break-up of a common parent body. From the current values of proper se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef4fc780c6afef533fba66618da3aa0a
https://doi.org/10.1016/s0019-1035(02)00062-3
https://doi.org/10.1016/s0019-1035(02)00062-3
Publikováno v:
Icarus. 157:155-172
Asteroid families are believed to originate by catastrophic disruptions of large asteroids. They are nowadays identified as clusters in the proper orbital elements space. The proper elements are analytically defined as constants of motion of a suitab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0968a8de75c882d467e2b9235b841e0f
https://doi.org/10.1006/icar.2002.6830
https://doi.org/10.1006/icar.2002.6830
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Context. It is widely accepted that the current distribution of material in the main asteroidal belt (MB) is a product of the evolutionary history of the solar system during its whole lifetime of ~4.5 billions of years and is, consequently, a major w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbd39db1cdd8c1aad1f3c377cdcf47c9
https://doi.org/10.1051/0004-6361/201525754
https://doi.org/10.1051/0004-6361/201525754
Autor:
David Vokrouhlický, Brian D. Warner, Petr Pravec, Kamil Hornoch, Peter Kusnirak, William F. Bottke, Josef Ďurech, J. Vrastil, Julian Oey, R. Groom
Publikováno v:
Astronomy & Astrophysics. 585:A56
Context. The low-albedo part of the Nysa-Polana-Hertha asteroid complex has recently been found to consist of at least two families. The larger of them has been associated with asteroid 495 Eulalia, hereafter named the Eulalia family. The unstable lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b5c382dc5a5496817e4b5b75bb32ab26
https://doi.org/10.1051/0004-6361/201526953
https://doi.org/10.1051/0004-6361/201526953
Autor:
Viktor Radović, B. Novakovic
Publikováno v:
Proceedings of the International Astronomical Union. 9:174-175
Introduction: Asteroid families are believed to have originated from catastrophic collisions among asteroids. They are a very important subject of Solar System investigation, because practically any research topic carried out in asteroid-related scie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::de2e6fcef182bd10c0a9824b8b73367b
https://doi.org/10.1017/s1743921314008187
https://doi.org/10.1017/s1743921314008187
Publikováno v:
Serbian Astronomical Journal
Serbian Astronomical Journal, Vol 179, Pp 75-86 (2009)
Serbian Astronomical Journal, Vol 2009, Iss 179, Pp 75-86 (2009)
Serbian Astronomical Journal, Vol 179, Pp 75-86 (2009)
Serbian Astronomical Journal, Vol 2009, Iss 179, Pp 75-86 (2009)
A procedure of gridification of the computation of asteroid proper orbital elements is described. The need to speed up the time consuming computations and make them more efficient is justified by the large increase of observational data expected from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59aacf34fb239d13a38674cc801a4a63
Asteroid families, traditionally defined as clusters of objects in orbital parameter space, often have distinctive optical colors. We show that the separation of family members from background interlopers can be improved with the aid of SDSS colors a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19f012735b97bc2f42a614d1b4b8681f
http://arxiv.org/abs/0807.3762
http://arxiv.org/abs/0807.3762
