Analysis of the Hungaria asteroid population

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F09%3A00207347" target="_blank" >RIV/00216208:11320/09:00207347 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Analysis of the Hungaria asteroid population

Original language description

There are approximately 5000 known asteroids in the Hungaria orbital space, a region defined by orbits with high inclination (16° { i { 34°), low eccentricities (e { 0.18), and semi-major axes 1.78 { a { 2.0 AU. We argue that this region is populated bya large number of asteroids formed after a catastrophic collision involving (434) Hungaria, the presumptive largest fragment of the Hungaria collisional family. The remaining objects form a background population that share orbital characteristics with the family members.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/GA205%2F08%2F0064" target="_blank" >GA205/08/0064: The Yarkovsky and YORP effects in translational and rotational dynamics of asteroids</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2009

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Icarus : International Journal of Solar System Studies

ISSN

0019-1035

e-ISSN

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Volume of the periodical

204

Issue of the periodical within the volume

1

Country of publishing house

MX - MEXICO

Number of pages

11

Pages from-to

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UT code for WoS article

000270884100012

EID of the result in the Scopus database

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